An optical spectroscopic HR diagram for low-mass stars and brown dwarfs in Orion

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...

Disgrifiad llawn

Manylion Llyfryddiaeth
Prif Awduron:	Riddick, F, Roche, P, Lucas, P
Fformat:	Journal article
Iaith:	English
Cyhoeddwyd:	2007

Eitemau Tebyg

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