The effective temperature scale of M dwarfs
Context. Despite their large number in the Galaxy, M dwarfs remain elusive objects and the modeling of their photosphere has long remained a challenge (molecular opacities, dust cloud formation). Aims. Our objectives are to validate the BT-Settl model atm
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
|01_Rajpurohit_The_effective_temperature_2013.pdf||1.3 MB||Adobe PDF|
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