Low-mass star formation in Lynds 1333

Details Low-mass star formation in Lynds 1333 Low-mass star formation in Lynds 1333

2006-06-20

arxiv.org/abs/astro-ph/0606471v1

Mon.Not.Roy.Astron.Soc.371:732-738,2006

Astronomy and Astrophysics

Astrophysics

7 pages, 4 figures, accepted by MNRAS

Scientific paper

10.1111/j.1365-2966.2006.10698.x

Medium-resolution optical spectroscopy of the candidate YSOs associated with the small, nearby molecular cloud Lynds~1333 revealed four previously unknown classical T Tauri stars, two of which are components of a visual double, and a Class I source, IRAS 02086+7600. The spectroscopic data, together with new V,R_ C,I_C photometric and 2MASS J, H, and K_s data allowed us to estimate the masses and ages of the new T Tauri stars. We touch on the possible scenario of star formation in the region. L1333 is one of the smallest and nearest known star forming clouds, therefore it may be a suitable target for studying in detail the small scale structure of a star forming environment.

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