The formation of low-mass stars

Details The formation of low-mass stars The formation of low-mass stars

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pasp..101..229w&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 101, March 1989, p. 229-243. Research supported by NASA

Astronomy and Astrophysics

Astronomy

17

Infrared Astronomy, Interstellar Matter, Molecular Clouds, Star Formation, Stellar Mass, Interstellar Gas, Ophiuchi Clouds, Spectral Energy Distribution, Stellar Luminosity, Taurus Constellation

Scientific paper

Visible to millimeter wavelength observations of the global and individual aspects of low-mass star formation are discussed. Infrared and millimeter-wave techniques reveal large collections of dust-embedded young stellar objects associated with the densest regions of molecular clouds. Special attention is given to studies of the Taurus-Auriga and Rho Opiuchi molecular cloud complexes. Properties such as the bolometric luminosities and evolutionary states of young objects can be determined by modeling the 1-100-micron spectral energy distributions.

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