An optical spectroscopic HR diagram for low-mass stars and brown dwarfs in Orion
The masses and temperatures of young low-mass stars and brown dwarfs in star-forming regions are not yet well established because of uncertainties in the age of individual objects and the spectral type-temperature scale appropriate for objects with ages of only a few Myr. Using multi-object optical...
| Κύριοι συγγραφείς: | , , |
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| Μορφή: | Journal article |
| Γλώσσα: | English |
| Έκδοση: |
2007
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