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Emission Lines from Superwinds of Super Star Clusters

Emission Lines from Superwinds of Super Star Clusters

Talk presented at American Astronomical Society (AAS) Winter 237st Virtual Meeting, USA, January 2021

Ashkbiz Danehkar

January 12, 2021
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  1. Ashkbiz Danehkar Department of Astronomy, University of Michigan [email protected] In

    Collaborations with: Sally Oey, and Will Gray 237th AAS Meeting, Virtually Anywhere, January 12th, 2021 Emission Lines from Superwinds of Super Star Clusters
  2. 2 Superwinds and Super Bubbles Schematic View of Superwind and

    Super Bubble (Romero+ 2018, Strickland+ 2003)
  3. 3 Catastrophic Cooling of Superwind NGC 2366 Green Pea analog!

    [O II], [O III] and Continuum (Oey+ 2017) Mrk 71 Oey + 2017
  4. 4 Superwind Theory  Adiabatic Solution – Chevalier & Clegg

    1985 – Without Radiative Cooling  Radiative Solution – Silich et al. 2004 – With Radiative Cooling Silich + 2004
  5. 9 Hydrodynamic Simulation of Superwinds Radiative Cooling  adiabatic (AC),

    adiabatic with bubble (AB),  catastrophic cooling (CC), catastrophic cooling the bubble (CB) Temperature discrepancy factor (fT = Trad / Tadi) Danehkar, Oey, Gray, 2021
  6. 16 Summary  Superwinds Theory  Without Radiative Cooling (Chevalier

    & Clegg 85)  With Radiative Cooling (Silich + 2004)  Superwind Suppression – Catastrophic Cooling (Gray, Oey, Silich, 2019) – Parametric Investigation (Danehkar, Oey, Gray, 2021)  Emission-line Predictions (Danehkar, Oey, Gray, 2021) – Emission flux calculated for adiabatic and cooling solutions – BPT & UV Diagnostic Diagrams