The environments of young stars - Mid-infrared and molecular line imaging

Details The environments of young stars - Mid-infrared and molecular line imaging The environments of young stars - Mid-infrared and molecular line imaging

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...401l.113k&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 401, no. 2, p. L113-L116.

Astronomy and Astrophysics

Astronomy

24

Early Stars, Infrared Astronomy, Massive Stars, Molecular Spectra, Star Formation, Emission Spectra, Interstellar Masers, Stellar Luminosity, Stellar Mass Accretion, Stellar Temperature

Scientific paper

Consideration is given to new high-resolution images of the regions W3(OH) and G34.3 + 0.1 in the mid-infrared made with the Berkeley mid-IR Array Camera and in NH3 line emission made with the VLA. The energy requirements of the H2O masers seen in faint cores in both star-forming regions suggest that both cores now contain stars. Our observations suggest that the stars are probably no earlier than type A and may be later if sources of energy such as accretion contribute to the luminosity.

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