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Intro talk K. A. Lutz

Katharina
March 29, 2020

Intro talk K. A. Lutz

Katharina

March 29, 2020
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  1. 30/03/20 K. Lutz - Intro to my Science 3 Katharina

    Schweinfurt Born & raised Munich (TUM & MPE) BSc: Novae in M31 with W. Pietsch, J. Greiner MSc: Metallicity gradients in xGASS galaxies with A. Saintonge, L. Tacconi Melbourne (SUT, CSIRO) PhD: HI in HI eXtreme galaxies, gas Kinematics, metallicities with V. Kilborn & B. Catinella Strasbourg (CDS, ObAS) Post-Doc: Scientific support of VO proects and all my favourite Science with CDS team, C. Bot, L. Posti, B. Vollmer
  2. 30/03/20 K. Lutz - Intro to my Science 4 My

    current position CDS postdoc Science Functional work
  3. 30/03/20 K. Lutz - Intro to my Science 5 Star

    formation – gas cycle Stars Old stars: Stellar winds Supernovae Accretion Star formation Cooling Condensation Dust Metals
  4. 30/03/20 K. Lutz - Intro to my Science 6 Science

    questions Where does the cold gas come from and where does it go? Catinella et al. (2018), Saintonge, …, Lutz et al. (2017)
  5. 30/03/20 K. Lutz - Intro to my Science 7 Science

    questions How are cold gas (HI and H 2 ), metallicity and dust correlated? Globally and locally? Bothwell et al. (2013)
  6. 30/03/20 K. Lutz - Intro to my Science 8 Science

    questions How does the angular momentum affect galaxy evolution? Maddox et al. (2015) Romanowsky & Fall (2012)
  7. 30/03/20 K. Lutz - Intro to my Science 9 All

    my science projects • xGASS & xCOLDGASS metallicity → metall gradients and cold gas • HIX HI-rich galaxies → metall • SHREG properties of resolved HI discs → metall • MCX SEDs between → metall μm and cm • AG/DC All gas and dust content of → metall galaxies
  8. 30/03/20 K. Lutz - Intro to my Science 10 XGASS

    / xCOLD GASS Lutz et al. (in prep.)
  9. 30/03/20 K. Lutz - Intro to my Science 11 XGASS

    / xCOLDGASS • Statistics are hard • Local metallicity correlates with global HI content (and not with H 2 )
  10. 30/03/20 K. Lutz - Intro to my Science 12 HIX

    galaxies – sample selection
  11. 30/03/20 K. Lutz - Intro to my Science 15 HIX

    galaxies – star formation Lutz et al. (2017)
  12. 30/03/20 K. Lutz - Intro to my Science 17 HIX

    galaxies – angular momentum Lutz et al. (2018)
  13. 30/03/20 K. Lutz - Intro to my Science 18 HIX

    galaxies – halo spin Lutz et al. (2018)
  14. 30/03/20 K. Lutz - Intro to my Science 19 HIX

    galaxies – gas-phase metallicity Lutz et al. (2020)
  15. 30/03/20 K. Lutz - Intro to my Science 20 HIX

    galaxies - outlook • Dust content from SED modelling • CO ALMA data
  16. 30/03/20 K. Lutz - Intro to my Science 21 HIX

    conclusion • HIX galaxies are HI rich and average star formers • HI disc as big as can be supported by specific angular momentum • Halo spin large – High angular momentum – Slow evolution
  17. 30/03/20 K. Lutz - Intro to my Science 24 SHREG

    conclusion • More than 600 HI data cubes • Kinematic modelling has begun • Angular momentum – mass relation surprisingly scattered
  18. 30/03/20 K. Lutz - Intro to my Science 26 MSX

    conclusion • IRAM proposal resubmitted with Caroline and Chris
  19. 30/03/20 K. Lutz - Intro to my Science 28 CDS

    service work • Virtual Observatory Tutorials – Python – Standard VO applications • Providing a scientists viewpoints on: – Radio data archives – Science Platforms