Four Probable T Tauri Stars in MBM 12

Details Four Probable T Tauri Stars in MBM 12 Four Probable T Tauri Stars in MBM 12

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pasj...55l..49o&link_type=abstract

Publications of the Astronomical Society of Japan, Vol.55, No.4, pp. L49-L52

Astronomy and Astrophysics

Astronomy

3

Ism: Individual (Mbm 12) -- Stars: Emission-Line -- Stars: Formation -- Stars: Pre-Main Sequence

Scientific paper

Survey observations were carried out in the MBM 12 (sometimes referred to as Lynds 1457) dark cloud in search of Hα emission stars by using a slitless grism spectrograph on the 2.6-m reflector of Byurakan Astrophysical Observatory, Armenia. Four new Hα stars were detected by the survey and identified as candidate T Tauri stars by follow-up low-dispersion spectroscopy and/or near-infrared photometry.

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