Two new T Tauri stars and a candidate FU Orionis star associated with BOK globules.

Details Two new T Tauri stars and a candidate FU Orionis star associated with BOK globules. Two new T Tauri stars and a candidate FU Orionis star associated with BOK globules.

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...320..167y&link_type=abstract

Astronomy and Astrophysics, v.320, p.167-171

Astronomy and Astrophysics

Astrophysics

20

Stars: Formation, Stars: Pre-Main-Sequence, Ism: Clouds, Ism: Individual: Cb 34, Infrared: Stars

Scientific paper

We present photometric and spectroscopic evidence of two new T Tauri stars formed in the conditions of isolated small Bok globules. The spectral energy distributions of these objects display excess infrared emission, they are associated with optical reflection nebulae, and their optical spectra reveal Balmer emission lines and the Li I λ6707Å absorption line. Additionally, we report the discovery of what may be a new FU Orionis star seen towards Bok globule CB 34. The star is about 4 magnitudes brighter than it appears on the Palomar plates and is associated with the aggregate of young stellar objects forming in Bok globule CB 34.

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