Implications of a Temperature Dependent IMF III: Mass Growth and Quiescence

Autor: Steinhardt, Charles L., Sneppen, Albert, Hensley, Hagan, Jermyn, Adam S., Mostafa, Basel, Weaver, John R., Brammer, Gabriel, Clark, Thomas H., Davidzon, Iary, Diaconu, Andrei C., Mobasher, Bahram, Rusakov, Vadim, Toft, Sune

The stellar initial mass function (IMF) is predicted to depend upon the temperature of gas in star-forming molecular clouds. The introduction of an additional parameter, $T_{IMF}$ , into photometric template fitting, suggest most galaxies obey an IMF

Externí odkaz: http://arxiv.org/abs/2206.01750

The Earliest Stage of Galactic Star Formation

Autor: Steinhardt, Charles L., Rusakov, Vadim, Clark, Thomas H., Diaconu, Andrei C., Forbes, John C., McPartland, Conor J. R., Sneppen, Albert, Weaver, John

Publikováno v: Steinhardt, C L, Rusakov, V, Clark, T H, Diaconu, A, Forbes, J, Mc Partland, C J R, Sneppen, A & Weaver, J 2023, ' The Earliest Stage of Galactic Star Formation ', Astrophysics Journal Letters, vol. 949, no. 2, L38 . https://doi.org/10.3847/2041-8213/acd447

Using a recently-developed technique to estimate gas temperatures ($T_\textrm{SF}$) in star-forming regions from large photometric surveys, we propose a diagram, analogous to the Hertzsprung-Russell diagram for individual stars, to probe the evolutio

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2ed3444ba4df53de3f67136f9bc79cd4
https://curis.ku.dk/portal/da/publications/the-earliest-stage-of-galactic-star-formation(39c54928-6520-4512-8687-1f83e31fb0b8).html