Star Formation, GMCs, and Galaxies

Add to your list(s) Download to your calendar using vCal

• Norm Murray (CITA)
• Thursday 24 January 2019, 16:00-17:00
• Sackler Lecture Theatre, IoA (tea at 3:30 pm).

If you have a question about this talk, please contact ma557.

Star formation on galactic scales is observed to be a slow process, a result known as the Kennicutt-Schmidt relation. I will argue, using observations, simulations, and analytic theory, that the star formation on smaller scales, those of Giant Molecular Clouds (GMCs), increases with GMC age. I will show, using a new GMC catalog, that GMCs in the “five kiloparsec ring” of the Milky Way are contracting under self-gravity, and argue that this collapse is halted and reversed by feedback from star clusters. I will then describe the results of the FIRE simulations, which show that in galaxies with higher gas surface density, and hence more massive GMCs, the feedback not only disrupts the GMCs, it drives winds from the simulated galaxies; at high redshifts, the simulated winds remove the interstellar medium of the galaxy, halting star formation for a dynamical time. Upcoming CO intensity mapping experiments will test this prediction of the FIRE simulations.

This talk is part of the Institute of Astronomy Colloquia series.

This talk is included in these lists:

• Cambridge Astronomy Talks
• Combined External Astrophysics Talks DAMTP
• Cosmology lists
• Cosmology, Astrophysics and General Relativity
• Institute of Astronomy Colloquia
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists
• Priscilla
• Sackler Lecture Theatre, IoA (tea at 3:30 pm)

Note that ex-directory lists are not shown.