From raffaella.schneider at roma1.infn.it  Sat May  1 15:09:39 2021
From: raffaella.schneider at roma1.infn.it (raffaella.schneider at roma1.infn.it)
Date: Sat, 1 May 2021 15:09:39 +0200
Subject: [astroseminar@Sapienza] astro seminar by Michele Ginolfi,
	thursday May 6 at 16:30
Message-ID: <B118A373-720A-4AF1-91AB-904923076008@roma1.infn.it>

Dear Colleagues,

I am pleased to announce the following astrophysics seminar to be held remotely on
Thursday May 6 at 16:30. Title, abstract and link details are given below.

Best regards

Raffaella Schneider



????
Thursday May 6 at 16:30

Michele Ginolfi (European Southern Observatory)

Galactic feedback and circumgalactic metal enrichment in the early Universe

Galaxies evolve under the influence of gas exchanges with their surrounding gaseous halos, the so-called circumgalactic medium (CGM), 
extending over tens of kpc. A solid characterisation of both galactic gas flows and chemical composition of the CGM is thus crucial to 
understand galaxy evolution, especially in the first few Gyrs of cosmic time, when galaxies rapidly assembled their masses and reached their chemical maturity.
I will present new studies on galactic outflows and CGM metal enrichment in the early Universe, exploiting recent data from the ALMA large program ALPINE, 
that observed [CII] and dust in more than hundred star-forming galaxies at z~4-6.

Link: https://uniroma1.zoom.us/j/85962662885?pwd=UDFLcTYrWHNSWm5uQ1ZrbEhsalVUUT09 <https://uniroma1.zoom.us/j/85962662885?pwd=UDFLcTYrWHNSWm5uQ1ZrbEhsalVUUT09>
????









-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists2.roma1.infn.it/pipermail/astroseminar/attachments/20210501/db7621b3/attachment.html 

From raffaella.schneider at roma1.infn.it  Thu May  6 16:01:54 2021
From: raffaella.schneider at roma1.infn.it (raffaella.schneider at roma1.infn.it)
Date: Thu, 6 May 2021 16:01:54 +0200
Subject: [astroseminar@Sapienza] astro seminar by Michele Ginolfi,
 thursday May 6 at 16:30
In-Reply-To: <B118A373-720A-4AF1-91AB-904923076008@roma1.infn.it>
References: <B118A373-720A-4AF1-91AB-904923076008@roma1.infn.it>
Message-ID: <987815C9-1E3F-4DBB-9DA3-1A94C93EC28C@roma1.infn.it>

Dear Colleagues, 

this is a gentle reminder for the astrophysics seminar starting in 30 minutes.

Best regards

Raffaella

Prof. Raffaella Schneider
Dipartimento di Fisica "G. Marconi?
Senior Fellow, Scuola Superiore di Studi Avanzati Sapienza
Sapienza, Universit? di Roma
P.le A. Moro 2, 00185 Roma, Italy


> On 1 May 2021, at 15:09, raffaella.schneider at roma1.infn.it wrote:
> 
> Dear Colleagues,
> 
> I am pleased to announce the following astrophysics seminar to be held remotely on
> Thursday May 6 at 16:30. Title, abstract and link details are given below.
> 
> Best regards
> 
> Raffaella Schneider
> 
> 
> 
> ????
> Thursday May 6 at 16:30
> 
> Michele Ginolfi (European Southern Observatory)
> 
> Galactic feedback and circumgalactic metal enrichment in the early Universe
> 
> Galaxies evolve under the influence of gas exchanges with their surrounding gaseous halos, the so-called circumgalactic medium (CGM), 
> extending over tens of kpc. A solid characterisation of both galactic gas flows and chemical composition of the CGM is thus crucial to 
> understand galaxy evolution, especially in the first few Gyrs of cosmic time, when galaxies rapidly assembled their masses and reached their chemical maturity.
> I will present new studies on galactic outflows and CGM metal enrichment in the early Universe, exploiting recent data from the ALMA large program ALPINE, 
> that observed [CII] and dust in more than hundred star-forming galaxies at z~4-6.
> 
> Link: https://uniroma1.zoom.us/j/85962662885?pwd=UDFLcTYrWHNSWm5uQ1ZrbEhsalVUUT09 <https://uniroma1.zoom.us/j/85962662885?pwd=UDFLcTYrWHNSWm5uQ1ZrbEhsalVUUT09>
> ????
> 
> 
> 
> 
> 
> 
> 
> 
> 
> _______________________________________________
> astroseminar mailing list
> astroseminar at roma1.infn.it
> https://lists2.roma1.infn.it/mailman/listinfo/astroseminar

-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists2.roma1.infn.it/pipermail/astroseminar/attachments/20210506/a796b1a6/attachment.html 

From paolo.pani at uniroma1.it  Fri May  7 15:11:07 2021
From: paolo.pani at uniroma1.it (Paolo Pani)
Date: Fri, 7 May 2021 15:11:07 +0200
Subject: [astroseminar@Sapienza] Gravity theory webinar Mon,
 May 10th @noon: Alexandre Toubiana (APC Paris) - "Modeling
 gravitational waves from exotic compact objects"
Message-ID: <CADjeKwAJQjwNh0vN_omHdpD7TRnEJcGHfpaiW+jpDMNmF+QeJg@mail.gmail.com>

Announcement of the next gravity-theory webinar:

*Alexandre Toubiana (APC Paris)** - "*Modeling gravitational waves from
exotic compact objects*"*
*Mon, May 10th @noon*

Abstract:

*In the standard astrophysical paradigm, the only compact objects (with
C>0.1) are black holes (BHs) and neutron stars (NSs). However, extensions
of General Relativity (GR) and/or of the Standard Model can give rise to
``exotic compact objects'' (ECOs), which mimic the gravitational behavior
of BHs and NSs to varying degrees. Thus, exotic compact objects can be
difficult to distinguish from BHs and NSs in the inspiral phase of the
binaries observed by gravitational-wave detectors, but significant
differences may be present in the merger and post-merger signal.In this
talk I will briefly review some models of ECOs and numerical simulations of
non-BH binaries. Based on these results, I will present a toy model aiming
to capture the main features of the full GW signal emitted by ECO binaries
and use it to assess the detectability of such exotic signals with current
and future detectors, and whether they can be distinguished from black hole
binaries.*

Zoom link:
https://uniroma1.zoom.us/j/81283707469?pwd=SzkyMk5jRm0xcEN3WE5MYVh1RVFtQT09
ID meeting: 812 8370 7469
Passcode: 915450

Have a nice weekend,
Paolo

-- 
Paolo Pani
Associate Professor
ERC StG Fellow, DarkGRA project
Junior Fellow, Scuola Superiore di Studi Avanzati Sapienza

Physics Department (Marconi Building), 3rd floor, room 334
Sapienza University of Rome
Piazzale Aldo Moro 5 - 00185 Rome (Italy)
+39 06 4991 4472 (int 24472)

-- 
________________________________________________________
Le informazioni 
contenute in questo messaggio di posta elettronica sono strettamente 
riservate e indirizzate esclusivamente al destinatario. Si prega di non 
leggere, fare copia, inoltrare a terzi o conservare tale messaggio se non 
si ? il legittimo destinatario dello stesso. Qualora tale messaggio sia 
stato ricevuto per errore, si prega di restituirlo al mittente e di 
cancellarlo permanentemente dal proprio computer.
The information contained 
in this e mail message is strictly confidential and intended for the use of 
the addressee only.? If you are not the intended recipient, please do not 
read, copy, forward or store it on your computer. If you have received the 
message in error, please forward it back to the sender and delete it 
permanently from your computer system.

-- 

Fai crescere i nostri giovani ricercatori
dona il?5?per?mille?alla 
Sapienza
*codice?fiscale?80209930587*

-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists2.roma1.infn.it/pipermail/astroseminar/attachments/20210507/21175fe6/attachment.html 

From raffaella.schneider at roma1.infn.it  Wed May 12 12:15:39 2021
From: raffaella.schneider at roma1.infn.it (raffaella.schneider at roma1.infn.it)
Date: Wed, 12 May 2021 12:15:39 +0200
Subject: [astroseminar@Sapienza] Announcement of the 5th Quid Ultra
 colloquium by Roberto Maiolino, May 18 2021 at 16:30
Message-ID: <18E024D9-01B0-45EE-AF76-A566D48CBEAE@roma1.infn.it>

Dear Colleagues,

we are pleased to announce that the fifth colloquium of the program QUID ULTRA? Frontiers and Controversies in Astrophysics, 
will be on May 18 2021 at 16:30 by Roberto Maiolino (Cavendish Laboratory, University of Cambridge).  Title and abstract
are attached below. 

The program QUID ULTRA? Frontiers and Controversies in Astrophysics is a series of monthly prestigious colloquia that will be 
running from early February till December 2021. This initiative has been funded by Sapienza University with the co-sponsorship of 
INAF/Astronomical Observatory of Rome and of the joint PhD program in Astronomy, Astrophysics and Space Science of Sapienza, 
Tor Vergata University and INAF.

Looking forward to seeing you soon, 

Raffaella Schneider (on behalf of the SOC)

Prof. Raffaella Schneider
Dipartimento di Fisica "G. Marconi?
Senior Fellow, Scuola Superiore di Studi Avanzati Sapienza
Sapienza, Universit? di Roma
P.le A. Moro 2, 00185 Roma, Italy
raffaella.schneider at uniroma1.it


????????????????
May 18 2021 at 16:30

Roberto Maiolino (Cavendish Laboratory, University of Cambridge)

Title: Quenching star formation in galaxies

Abstract: 
In the local universe stars only make up about 7% of all baryons, indicating that star formation has been extremely inefficient 
across the cosmic epochs. Within this context, even more impressive is the fact that in a significant fraction of galaxies star 
formation has been totally ?quenched?, resulting into the population of passive and quiescent local galaxies. Understanding 
what are the mechanisms responsible for suppressing or even quenching star formation in galaxies has been one of the main 
challenges of astrophysics in recent years and it is one of the research areas in which most of the efforts have been directed, 
both in terms of cosmological simulations and in terms of observing campaigns.
I will give an overview of the potential causes and physical processes that might be responsible for regulating or even 
leading to the complete suppression of star formation in galaxies. I will illustrate that there are a variety of possible culprits. 
Among these I will show that supernova explosions can play a role, but the energy injected in the interstellar and intergalactic 
medium by accreting supermassive black holes can have a truly dramatic effect on their host galaxies. The environment in 
which galaxies live (e.g. galaxy groups or clusters) can also play an important role, by suppressing star formation especially 
in satellite galaxies. I will discuss observational evidence for these various effects by using results from extensive 
multi-wavelength datasets. I will conclude by emphasizing open, outstanding problems and the possibility of tackling them 
with the next generation of observing facilities.

Join Zoom Meeting
https://uniroma1.zoom.us/j/89931306878?pwd=WG5RYlYyZzRSMzJsOFpSRHczWEFCZz09 <https://uniroma1.zoom.us/j/89931306878?pwd=WG5RYlYyZzRSMzJsOFpSRHczWEFCZz09>

Meeting ID: 899 3130 6878
Passcode: 419276
????????????????











-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists2.roma1.infn.it/pipermail/astroseminar/attachments/20210512/23de80d1/attachment.html 

From raffaella.schneider at roma1.infn.it  Sun May 16 23:10:31 2021
From: raffaella.schneider at roma1.infn.it (raffaella.schneider at roma1.infn.it)
Date: Sun, 16 May 2021 23:10:31 +0200
Subject: [astroseminar@Sapienza] Amaldi Research Center seminar - Prof.
 Michela Mapelli, thursday 20/05/2021 at 16:00
Message-ID: <83B5B93E-29BE-489D-8A69-5818F9754A3A@roma1.infn.it>

Dear Colleagues,

I am pleased to announce the following seminar of the Amaldi Research Center.

Best regards,

Raffaella Schneider

Prof. Raffaella Schneider
Dipartimento di Fisica "G. Marconi?
Senior Fellow, Scuola Superiore di Studi Avanzati Sapienza
Sapienza, Universit? di Roma
P.le A. Moro 2, 00185 Roma, Italy
raffaella.schneider at uniroma1.it

??????????
Amaldi Research Center seminar

Thursday May 20 2021, 4 pm

Prof. Michela Mapelli (Universit? di Padova)

Title: "Binary black holes and intermediate-mass black holes across cosmic time?

Abstract:

The latest results from the LIGO-Virgo-KAGRA collaboration draw a spectacular fresco of binary black hole mergers, ranging from a few to more than hundred solar masses. In this talk, I will discuss the main astrophysical formation channels of binary black holes, highlighting the open questions. On the one hand, models of stellar evolution and pair instability suggest the existence of a gap in the mass spectrum of black holes between ~60 and ~120 solar masses. The boundaries of this gap drastically depend on stellar rotation and on the efficiency of envelope removal. On the other hand, extreme dynamical processes in dense star clusters can fill the mass gap, via multiple stellar collisions, dynamical exchanges and hierarchical mergers. These processes might build up intermediate-mass black holes with mass up to several thousand solar masses, especially in the most metal-poor and massive clusters. The evolution of such dynamical mergers across cosmic time will be one of the most exciting targets of next-generation ground-based detectors.
??????????









-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists2.roma1.infn.it/pipermail/astroseminar/attachments/20210516/c2446283/attachment.html 

From raffaella.schneider at roma1.infn.it  Sun May 16 23:15:14 2021
From: raffaella.schneider at roma1.infn.it (raffaella.schneider at roma1.infn.it)
Date: Sun, 16 May 2021 23:15:14 +0200
Subject: [astroseminar@Sapienza] ARC seminar by Michela Mapelli - zoom link!
Message-ID: <6203E1CE-6413-4267-9FBD-A780B835AA2A@roma1.infn.it>

Dear Colleagues,

I apologize, here is the announcement with the zoom link information.

Best regards

Raffaella 

Prof. Raffaella Schneider
Dipartimento di Fisica "G. Marconi?
Senior Fellow, Scuola Superiore di Studi Avanzati Sapienza
Sapienza, Universit? di Roma
P.le A. Moro 2, 00185 Roma, Italy
raffaella.schneider at uniroma1.it


??????????
Amaldi Research Center seminar

Thursday May 20 2021, 4 pm

Prof. Michela Mapelli (Universit? di Padova)

Title: "Binary black holes and intermediate-mass black holes across cosmic time?

Abstract:

The latest results from the LIGO-Virgo-KAGRA collaboration draw a spectacular fresco of binary black hole mergers, ranging from a few to more than hundred solar masses. In this talk, I will discuss the main astrophysical formation channels of binary black holes, highlighting the open questions. On the one hand, models of stellar evolution and pair instability suggest the existence of a gap in the mass spectrum of black holes between ~60 and ~120 solar masses. The boundaries of this gap drastically depend on stellar rotation and on the efficiency of envelope removal. On the other hand, extreme dynamical processes in dense star clusters can fill the mass gap, via multiple stellar collisions, dynamical exchanges and hierarchical mergers. These processes might build up intermediate-mass black holes with mass up to several thousand solar masses, especially in the most metal-poor and massive clusters. The evolution of such dynamical mergers across cosmic time will be one of the most exciting targets of next-generation ground-based detectors.

zoom link:
https://uniroma1.zoom.us/j/89616189344?pwd=QlE0M0g1amh2aUMzWVh5alhxSjcvUT09 <https://uniroma1.zoom.us/j/89616189344?pwd=QlE0M0g1amh2aUMzWVh5alhxSjcvUT09> Meeting ID: 896 1618 9344 Passcode: 107157
??????????








-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists2.roma1.infn.it/pipermail/astroseminar/attachments/20210516/ef6c030b/attachment.html 

From raffaella.schneider at roma1.infn.it  Tue May 18 09:30:08 2021
From: raffaella.schneider at roma1.infn.it (raffaella.schneider at roma1.infn.it)
Date: Tue, 18 May 2021 09:30:08 +0200
Subject: [astroseminar@Sapienza] Gentle Reminder: Fifth online QUID ULTRA
 colloquium by Roberto Maiolino, today at 16:30
Message-ID: <F79759D1-F08C-4E48-94CE-B755740570A0@roma1.infn.it>

Dear Colleagues,

this is to gently remind you that the fifth online colloquium of the series: 

Quid Ultra? Frontiers and Controversies in Astrophysics 

will be today at 16:30. You can find all the details below and the updated program 
for future colloquia at the link:  https://www.quidultra.it <https://www.quidultra.it/>

Looking forward to seeing you soon, 

Raffaella Schneider (on behalf of the SOC)
  
Prof. Raffaella Schneider
Dipartimento di Fisica "G. Marconi?
Senior Fellow, Scuola Superiore di Studi Avanzati Sapienza
Sapienza, Universit? di Roma
P.le A. Moro 2, 00185 Roma, Italy
raffaella.schneider at roma1.infn.it <mailto:raffaella.schneider at roma1.infn.it>

????????????????
May 18 2021 at 16:30

Roberto Maiolino (Cavendish Laboratory, University of Cambridge)

Title: Quenching star formation in galaxies

Abstract: 
In the local universe stars only make up about 7% of all baryons, indicating that star formation has been extremely inefficient 
across the cosmic epochs. Within this context, even more impressive is the fact that in a significant fraction of galaxies star 
formation has been totally ?quenched?, resulting into the population of passive and quiescent local galaxies. Understanding 
what are the mechanisms responsible for suppressing or even quenching star formation in galaxies has been one of the main 
challenges of astrophysics in recent years and it is one of the research areas in which most of the efforts have been directed, 
both in terms of cosmological simulations and in terms of observing campaigns.
I will give an overview of the potential causes and physical processes that might be responsible for regulating or even 
leading to the complete suppression of star formation in galaxies. I will illustrate that there are a variety of possible culprits. 
Among these I will show that supernova explosions can play a role, but the energy injected in the interstellar and intergalactic 
medium by accreting supermassive black holes can have a truly dramatic effect on their host galaxies. The environment in 
which galaxies live (e.g. galaxy groups or clusters) can also play an important role, by suppressing star formation especially 
in satellite galaxies. I will discuss observational evidence for these various effects by using results from extensive 
multi-wavelength datasets. I will conclude by emphasizing open, outstanding problems and the possibility of tackling them 
with the next generation of observing facilities.

Join Zoom Meeting
https://uniroma1.zoom.us/j/89931306878?pwd=WG5RYlYyZzRSMzJsOFpSRHczWEFCZz09 <https://uniroma1.zoom.us/j/89931306878?pwd=WG5RYlYyZzRSMzJsOFpSRHczWEFCZz09>

Meeting ID: 899 3130 6878
Passcode: 419276
????????????????










-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists2.roma1.infn.it/pipermail/astroseminar/attachments/20210518/965a22fb/attachment.html 

From raffaella.schneider at roma1.infn.it  Tue May 18 16:30:23 2021
From: raffaella.schneider at roma1.infn.it (raffaella.schneider at roma1.infn.it)
Date: Tue, 18 May 2021 16:30:23 +0200
Subject: [astroseminar@Sapienza] new link zoom for  the quid ultra seminar
Message-ID: <F37E97FC-A3B2-4667-851B-364F131C48E7@roma1.infn.it>

Dear All,

due to technical difficulties we  had to change the original zoom link to this new one:

https://uniroma1.zoom.us/j/83598894783?pwd=NTBKeTZ2cU4vRW5xdVc4NDNpVDlidz09 <https://uniroma1.zoom.us/j/83598894783?pwd=NTBKeTZ2cU4vRW5xdVc4NDNpVDlidz09>

We apologize for the inconvenience,

See you soon

Raffaella



Prof. Raffaella Schneider
Dipartimento di Fisica "G. Marconi?
Senior Fellow, Scuola Superiore di Studi Avanzati Sapienza
Sapienza, Universit? di Roma
P.le A. Moro 2, 00185 Roma, Italy
raffaella.schneider at uniroma1.it
Phone: +39 06 4991 4312
Skype: raffasch
https://uniroma1.zoom.us/j/86939793732
Passcode: 789846










-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists2.roma1.infn.it/pipermail/astroseminar/attachments/20210518/a214b749/attachment.html 

From raffaella.schneider at roma1.infn.it  Wed May 19 23:46:33 2021
From: raffaella.schneider at roma1.infn.it (raffaella.schneider at roma1.infn.it)
Date: Wed, 19 May 2021 23:46:33 +0200
Subject: [astroseminar@Sapienza] gentle reminder - ARC seminar by Michela
 Mapelli, thursday May 20 at 4 pm
Message-ID: <AF6505C4-8DAC-4EBE-A898-38AB2DD6A090@roma1.infn.it>

Dear Colleagues,

this is a gentle reminder for the ARC seminar by Michela Mapelli. 
Details are given below,

Best regards

Raffaella


Prof. Raffaella Schneider
Dipartimento di Fisica "G. Marconi?
Senior Fellow, Scuola Superiore di Studi Avanzati Sapienza
Sapienza, Universit? di Roma
P.le A. Moro 2, 00185 Roma, Italy
raffaella.schneider at uniroma1.it

????????
Amaldi Research Center seminar

Thursday May 20 2021, 4 pm

Prof. Michela Mapelli (Universit? di Padova)

Title: "Binary black holes and intermediate-mass black holes across cosmic time?

Abstract:

The latest results from the LIGO-Virgo-KAGRA collaboration draw a spectacular fresco of binary black hole mergers, ranging from a few to more than hundred solar masses. In this talk, I will discuss the main astrophysical formation channels of binary black holes, highlighting the open questions. On the one hand, models of stellar evolution and pair instability suggest the existence of a gap in the mass spectrum of black holes between ~60 and ~120 solar masses. The boundaries of this gap drastically depend on stellar rotation and on the efficiency of envelope removal. On the other hand, extreme dynamical processes in dense star clusters can fill the mass gap, via multiple stellar collisions, dynamical exchanges and hierarchical mergers. These processes might build up intermediate-mass black holes with mass up to several thousand solar masses, especially in the most metal-poor and massive clusters. The evolution of such dynamical mergers across cosmic time will be one of the most exciting targets of next-generation ground-based detectors.

zoom link:
https://uniroma1.zoom.us/j/89616189344?pwd=QlE0M0g1amh2aUMzWVh5alhxSjcvUT09 <https://uniroma1.zoom.us/j/89616189344?pwd=QlE0M0g1amh2aUMzWVh5alhxSjcvUT09> Meeting ID: 896 1618 9344 Passcode: 107157
??????????













-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists2.roma1.infn.it/pipermail/astroseminar/attachments/20210519/400c44f8/attachment.html 

From raffaella.schneider at roma1.infn.it  Tue May 25 10:02:43 2021
From: raffaella.schneider at roma1.infn.it (raffaella.schneider at roma1.infn.it)
Date: Tue, 25 May 2021 10:02:43 +0200
Subject: [astroseminar@Sapienza] Announcement of the 6th QUID ULTRA
 colloquium by Debora Sijacki, 1 June at 16:30
Message-ID: <84715168-F2C5-492C-B5EE-558656C33037@roma1.infn.it>

Dear Colleagues,

we are pleased to announce that the sixth colloquium of the program QUID ULTRA? Frontiers and Controversies in Astrophysics, 
will be on June1 2021 at 16:30 by Debora Sijacki (Institute of Astronomy, University of Cambridge).  Title and abstract
are attached below. 

The program QUID ULTRA? Frontiers and Controversies in Astrophysics is a series of monthly prestigious colloquia that will be 
running from early February till December 2021. This initiative has been funded by Sapienza University with the co-sponsorship of 
INAF/Astronomical Observatory of Rome and of the joint PhD program in Astronomy, Astrophysics and Space Science of Sapienza, 
Tor Vergata University and INAF.

Looking forward to seeing you soon, 

Raffaella Schneider (on behalf of the SOC)

????????????????
June 1 2021 at 16:30

Debora Sijacki (Institute of Astronomy, University of Cambridge)

Title: The evolution of massive black holes through cosmic times?

Abstract: 
In this talk I will review current theoretical efforts in understanding supermassive black hole formation, accretion and feedback throughout cosmic time. Specifically, I will discuss possible links between large scale cosmological environments and supermassive black hole assembly and outline several possible interaction channels between active black holes and their host galaxies. In the second part of the talk I will focus on novel computational methods that allow us to follow black hole physics on much smaller scales in full galaxy formation simulations to unravel how black hole mass and spin evolve during the binary hardening stages or during launching of powerful jets.

Join Zoom Meeting
https://uniroma1.zoom.us/j/83598894783?pwd=NTBKeTZ2cU4vRW5xdVc4NDNpVDlidz09 <https://uniroma1.zoom.us/j/83598894783?pwd=NTBKeTZ2cU4vRW5xdVc4NDNpVDlidz09>

Meeting ID: 835 9889 4783
Passcode: 358787
????????????????







-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists2.roma1.infn.it/pipermail/astroseminar/attachments/20210525/8128d24d/attachment.html 

