Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Salim, Diane"'
Autor:
Alatalo, Katherine, Petric, Andreea O., Lanz, Lauranne, Rowlands, Kate, U, Vivian, Larson, Kirsten L., Armus, Lee, Barcos-Muñoz, Loreto, Evans, Aaron S., Koda, Jin, Luo, Yuanze, Medling, Anne M., Nyland, Kristina E., Otter, Justin A., Patil, Pallavi, Peñaloza, Fernando, Salim, Diane, Sanders, David B., Sazonova, Elizaveta, Skarbinski, Maya, Song, Yiqing, Treister, Ezequiel, Urry, C. Meg
We present the CO(1-0) maps of 28 infrared-bright galaxies from the Great Observatories All-Sky Luminous Infrared Galaxy Survey (GOALS) taken with the Combined Array for Research in Millimeter Astronomy (CARMA). We detect 100GHz continuum in 16 of 28
Externí odkaz:
http://arxiv.org/abs/2409.09116
Advancing our understanding of astrophysical turbulence is bottlenecked by the limited resolution of numerical simulations that may not fully sample scales in the inertial range. Machine learning (ML) techniques have demonstrated promise in up-scalin
Externí odkaz:
http://arxiv.org/abs/2307.02674
The physics regulating star formation (SF) in Hickson Compact Groups (HCG) has thus far been difficult to describe, due to their unique kinematic properties. In this study we expand upon previous works to devise a more physically meaningful SF relati
Externí odkaz:
http://arxiv.org/abs/2003.10458
Autor:
Jin, Keitaro, Salim, Diane M., Federrath, Christoph, Tasker, Elizabeth J., Habe, Asao, Kainulainen, Jouni T.
We determine the physical properties and turbulence driving mode of molecular clouds formed in numerical simulations of a Milky Way-type disc galaxy with parsec-scale resolution. The clouds form through gravitational fragmentation of the gas, leading
Externí odkaz:
http://arxiv.org/abs/1703.09709
Autor:
Federrath, Christoph, Salim, Diane M., Medling, Anne M., Davies, Rebecca L., Yuan, Tiantian, Bian, Fuyan, Groves, Brent A., Ho, I-Ting, Sharp, Robert, Kewley, Lisa J., Sweet, Sarah M., Richards, Samuel N., Bryant, Julia J., Brough, Sarah, Croom, Scott, Scott, Nicholas, Lawrence, Jon, Konstantopoulos, Iraklis, Goodwin, Michael
Stars form in cold molecular clouds. However, molecular gas is difficult to observe because the most abundant molecule (H2) lacks a permanent dipole moment. Rotational transitions of CO are often used as a tracer of H2, but CO is much less abundant a
Externí odkaz:
http://arxiv.org/abs/1703.09224
Akademický článek
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Whilst the star formation rate (SFR) of molecular clouds and galaxies is key in understanding galaxy evolution, the physical processes which determine the SFR remain unclear. This uncertainty about the underlying physics has resulted in various diffe
Externí odkaz:
http://arxiv.org/abs/1505.03144
Autor:
Keitaro Jin, Salim, Diane M., Federrath, Christoph, Tasker, Elizabeth J., Asao Habe, Kainulainen, Jouni T.
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Jul2017, Vol. 469 Issue 1, p383-393, 11p
Publikováno v:
Proceedings of the International Astronomical Union. Aug2015, Vol. 11 Issue A29B, p740-740. 1p.