UBV photometry in the vicinity of L379

Details UBV photometry in the vicinity of L379 UBV photometry in the vicinity of L379

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...94..265l&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 94, no. 2, Aug. 1992, p. 265-271.

Astronomy and Astrophysics

Astrophysics

8

Astronomical Catalogs, Astronomical Photometry, Interstellar Matter, Molecular Flow, Ubv Spectra, Data Reduction, Main Sequence Stars, Star Distribution, Stellar Luminosity, Stellar Magnitude

Scientific paper

UBV photometric sequence is presented for 102 stars in the vicinity of L379, which was obtained for distance determinations of L379, an isolated dark cloud which has been identified as a source of bipolar molecular flow. Of these stars, 76 are those with known MK spectral types. The available data were insufficient for an accurate distance determination of L379, and additional UBV photometry within the cloud is planned.

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