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...

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Bibliografski detalji
Glavni autori: Riddick, F, Roche, P, Lucas, P
Format: Journal article
Jezik:English
Izdano: 2007

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