Four Probable T Tauri Stars in MBM 12
Survey observations were carried out in the MBM 12 (sometimes referred to as Lynds 1457) dark cloud in search of $\mathrm{H}\alpha$ emission stars by using a slitless grism spectrograph on the 2.6-m reflector of Byurakan Astrophysical Observatory, Armenia. Four new $\mathrm{H}\alpha$ stars were dete...
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| Veröffentlicht in: | Publications of the Astronomical Society of Japan 2003-08, Vol.55 (4), p.L49-L52 |
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| Hauptverfasser: | , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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| Zusammenfassung: | Survey observations were carried out in the MBM 12 (sometimes referred to as Lynds 1457) dark cloud in search of
$\mathrm{H}\alpha$
emission stars by using a slitless grism spectrograph on the 2.6-m reflector of Byurakan Astrophysical Observatory, Armenia. Four new
$\mathrm{H}\alpha$
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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| ISSN: | 0004-6264 2053-051X |
| DOI: | 10.1093/pasj/55.4.L49 |