A low-luminosity far infrared source in the L1551 molecular cloud

Details A low-luminosity far infrared source in the L1551 molecular cloud A low-luminosity far infrared source in the L1551 molecular cloud

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....91l...1f&link_type=abstract

Astronomy and Astrophysics, vol. 91, no. 1-2, Nov. 1980, p. L1, L2. Swedish Board for Space Activities

Astronomy and Astrophysics

Astrophysics

43

Far Infrared Radiation, Main Sequence Stars, Molecular Clouds, Stellar Evolution, Stellar Luminosity, Gas Density, Near Infrared Radiation, Point Sources

Scientific paper

Searches at 85 and 150 microns of the molecular cloud L 1551 have
resulted in the discovery of an embedded source of total luminosity
approximately 25 solar luminosities. Its position coincides with an
obscured, near-infrared point source and with a gas density peak. It is
suggested that the embedded object is a low-mass pre-main-sequence star.

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