A survey of emission-line stars in the CMa star formation region

Details A survey of emission-line stars in the CMa star formation region A survey of emission-line stars in the CMa star formation region

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..311w&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

2

H Alpha Line, Line Spectra, Star Formation, Stellar Spectrophotometry, Ubv Spectra, T Tauri Stars

Scientific paper

A survey of emission-line stars was carried out in the CMa star formation region, based on spectral observations with the Kiso Schmidt telescope. In total, 128 emission-line stars were detected, ranging from V = 6 to 15, and the majority are found with V between 11 and 14. A comparison with the existing catalogues shows that some emission-line stars are common with ours, while some exhibit no detectable emission line on our plates, suggesting the variability of emission-line strength. The two-colour (U - B, B - V) diagram is also shown for the detected stars

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