Hertzsprung-Russell (H-R) diagram

Hertzsprung-Russell (H-R) diagram for previously know late-type objects in star forming region Chamaeleon I (from Luhman 2004) and the new member OTS 44 (black triangle in lower right of diagram). The solid lines are models of late-objects (very low mass stars and brown dwarfs) of different mass (dotted lines) in solar mass, and of different ages (solid) line in millions of years. OTS 44 correspond to a mass of about 0.015 Msun.

Créditos:

International Gemini Observatory/NOIRLab/NSF/AURA/

About the Image

Id:geminiann04018b
Tipo:Chart
Release date:30 de Noviembre de 2004 a las 05:00
Related announcements:geminiann04018
Size:500 x 500 px

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Categoría:Illustrations

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