A Parameter Study of the Dust and Gas Temperature in a Field of Young Stars
Autor: | Urban, Andrea, Evans II, Neal J., Doty, Steven D. |
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Rok vydání: | 2007 |
Předmět: | |
Zdroj: | Astrophys.J.698:1341-1356,2009 |
Druh dokumentu: | Working Paper |
DOI: | 10.1088/0004-637X/698/2/1341 |
Popis: | We model the thermal effect of young stars on their surrounding environment in order to understand clustered star formation. We take radiative heating of dust, dust-gas collisional heating, cosmic-ray heating, and molecular cooling into account. Using Dusty, a spherical continuum radiative transfer code, we model the dust temperature distribution around young stellar objects with various luminosities and surrounding gas and dust density distributions. We have created a grid of dust temperature models, based on our modeling with Dusty, which we can use to calculate the dust temperature in a field of stars with various parameters. We then determine the gas temperature assuming energy balance. Our models can be used to make large-scale simulations of clustered star formation more realistic. Comment: 29 pages, 19 figures. Submitted to ApJ |
Databáze: | arXiv |
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