New probable members of the young Orion stellar population. I - The obscured regions in Cassiopeia, VELA and Scorpius

Details New probable members of the young Orion stellar population. I - The obscured regions in Cassiopeia, VELA and Scorpius New probable members of the young Orion stellar population. I - The obscured regions in Cassiopeia, VELA and Scorpius

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...95..391m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 95, no. 3, p. 391-396.

Astronomy and Astrophysics

Astronomy

2

Early Stars, H Alpha Line, Sky Surveys (Astronomy), Astronomical Catalogs, Balmer Series, Emission Spectra

Scientific paper

Results are reported of a reinspection of H-alpha and direct plates taken at earlier epochs of obscured regions in the Cassiopeia, Vela, and Scorpius constellations. It was found that 43 new objects associated with obscured sky regions in the three constellations have their Balmer H-alpha line conspicuous (13), weak (13), or probably (17) in emission. This makes these objects good candidates to be members of the young Orion stellar population.

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