RU-D: "From the Large-Scale Structure to Galaxies, Stars and Planets" Science Day of the ORIGINS Excellence Cluster

Europe/Berlin
E.0.11 (MPA Large Seminar Room)

E.0.11

MPA Large Seminar Room

Karl-Schwarzschild-Straße 1, 85748 Garching bei München
Cesar Hernandez-Aguayo (MPA) , Maryam Arabsalmani (ORIGINS) , Milena Valentini (USM/LMU)
Description

RU-D annual meeting to address the milestones of the projects and to encourage further collaborations. Key speakers include Eric Emsellem (ESO), Thorsten Naab (MPA), Mathias Klein (USM/LMU) and Rolf Kudritzki (USM/LMU). The LOC is made up of Maryam Arabsalmani (Vera Rubin Fellow), Milena Valentini (Alexander von Humboldt Fellow at USM/LMU), Cesar Hernandez-Aguayo (ORIGINS postdoc at MPA), and the RU-D Coordinators, Volker Springel and Andreas Burkert. 


For remote access and to join the live-stream:
https://tum-conf.zoom.us/j/64293687766

Meeting ID: 642 9368 7766
Passcode: 125180


The timetable is loosely arranged according to the subareas of RU-D. There are slots for both 30 min (25 + 5 ) and 20 min (15 +5) talks.

  1. Galaxies in transition to extreme environments
  2. Formation and evolution of galaxies at the peak epoch of cosmic star formation
  3. The chemical and dynamical evolution of galaxies
  4. Understanding the physics of star formation
  5. Formation and characterization of planetary systems and their atmospheres
  6. The Cosmological ORIGINS Simulation Project

 

NEW MPA building access rules and corona measures:

  • Entry to the MPA building is only allowed for people who are either fully vaccinated against the corona virus, have recovered from a corona infection, or have tested negative against the corona virus in the last 24 hours (PCR or antigen corona test).
  • Participants have to confirm compliance with the building access rule via signature upon arrival, and as external visitors they have to be prepared to prove their vaccination, test, or recovery status by showing the corresponding certificates. Please bring your digital vaccination, recovery or test certificate, otherwise you can only participate via Zoom.
  • Mask wearing is strictly required in the seminar room if the 1.5 meter distance rule is not fulfilled or when not seated.
  • The mask-wearing mandate and social distancing in the hallways of MPA, and the recommendation for frequent hand sanitation, stay in place.
Participants
  • Alex Barreira
  • Alice Smith-Gicklhorn
  • Andreas Burkert
  • Barbara Ercolano
  • Cesar Hernandez-Aguayo
  • Claudia Pulsoni
  • Daniel Hernandez
  • Elena Hoemann
  • Eric Emsellem
  • Hans-Thomas Janka
  • Julien Wolf
  • Leonardo Testi
  • Luca Sala
  • Mara Salvato
  • Marina Ricci
  • Maryam Arabsalmani
  • Matthias Klein
  • Matthias Meier
  • Michael Hilker
  • Michael Weber
  • Milena Valentini
  • Ortwin Gerhard
  • Peter Ring
  • Rob Ivison
  • Roberto Saglia
  • Roland Triay
  • Rolf Kudritzki
  • Samuel Ward
  • Stefan Heigl
  • Thomas Preibisch
  • Thorsten Naab
  • Til Birnstiel
  • Vincenzo Mainieri
  • Volker Springel
Alice M. Smith-Gicklhorn, Science Manager
    • 09:00 09:10
      Welcome and Introduction - Volker Springel (Chair of Morning Session) and Andreas Burkert (Chair of Afternoon Session) 10m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
    • 09:10 09:20
      Today's and Tomorrow's Workspace 10m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Alice Smith-Gicklhorn (Excellence Cluster ORIGINS)
    • 09:20 09:50
      Star formation and multi-scale physics in disc galaxies: the PHANGS perspective 30m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Eric Emsellem
    • 09:50 10:10
      Merging filaments: A race against collapse 20m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Elena Hoemann
    • 10:10 10:30
      The impact of magnetic fields on protostellar mass accretion 20m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Stefan Heigl
    • 10:30 10:50
      Massive star explosions and large-scale galaxy dynamics 20m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München

      Abstract: Gamma Ray Bursts (GRBs), commonly associated with Broad-Line supernovae type Ic (SNe Ic-BL), and Super Luminous Supernovae (SLSNe) are the brightest astronomical phenomena in the Universe, located in hearts of star-forming regions. These violent explosions not only are valuable laboratories for extreme physical conditions, but also are powerful tracers of fundamental processes in galaxy formation and evolution. Although the link between GRBs/SLSNe and massive stars is well established, the physical properties of the stellar population that gives rise to these rare explosions and the interstellar medium conditions in which they form remain poorly constrained. Our recent studies indicate a possible link between rare galaxy dynamics and the formation of massive star progenitors of these violent events. If this be the case, the extreme conditions induced by galaxy dynamics (due to external/internal effects) could be the factors singling out the environment in which these bright transients form. The large-scale galaxy dynamics can be traced through the distribution and kinematics of neutral gas. I will describe our ongoing survey of neutral gas in z < 0.1 host galaxies, designed to investigate the structure of gas in the close environment of SNe Ic-BL / GRBs / SLSNe, and to explore the extreme conditions responsible for the formation of the progenitors of these explosions. I will in particular focus on our findings for the host galaxies of SN 1998bw / GRB 980425, SN 2017iuk / GRB 171205A, SLSN PTF10tpz, and AT2018cow, studied as a part of this survey, supporting the likely connection between massive star explosions and peculiar dynamics. Such a connection being commonplace will set these energetic transients as tracers of galaxies with extreme dynamics and also will help improve our understanding of the progenitor stars of these events.

      Speaker: Maryam Arabsalmani
    • 10:50 11:00
      Coffee break 10m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
    • 11:00 11:30
      The impact of merging supermassive black holes on the internal structure of massive galaxies 30m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Thorsten Naab
    • 11:30 11:50
      Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies 20m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Samuel Ruthven Ward
    • 11:50 12:10
      Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time 20m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Milena Valentini
    • 12:10 12:30
      Simulations of galaxy formation in the brane world 20m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Cesar Hernandez-Aguayo
    • 12:30 13:30
      Lunch at IPP's Kochmanufaktor 1h IPP

      IPP

      Boltzmannstraße 2
    • 13:30 14:00
      Galaxy Evolution and Metallicity: Simple Evolution Models vs. Observations & Cosmological Simulations 30m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Rolf Kudritzki
    • 14:00 14:20
      X-ray photoevaporation and the evolution of embedded giant planets 20m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Michael Weber
    • 14:20 14:40
      Recent advances in studying the galaxy-environment connection on large scales 20m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Alexandre Barreira
    • 14:40 15:00
      The stellar halo of massive early type galaxies 20m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Claudia Pulsoni
    • 15:00 15:15
      Coffee break 15m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
    • 15:15 15:45
      A multi-frequency view on the eROSITA final equatorial depth survey (eFEDS) 30m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Matthias Klein
    • 15:45 16:05
      Multi-wavelength analyses of galaxy clusters: from individual systems to large surveys 20m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Marina Ricci
    • 16:05 16:25
      Galaxy population in SPT galaxy clusters: the impact of cluster mergers 20m E.0.11

      E.0.11

      MPA Large Seminar Room

      Karl-Schwarzschild-Straße 1, 85748 Garching bei München
      Speaker: Daniel Hernandez-Lang
    • 16:25 16:35
      Closing Remarks - Volker Springel and Andreas Burkert 10m
    • 16:35 19:35
      Social gathering & informal discussions 3h

      MPA garden or indoors at MPA