A Second Phase of Star Formation in the Serpens Core

Details A Second Phase of Star Formation in the Serpens Core A Second Phase of Star Formation in the Serpens Core

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...275..195c&link_type=abstract

Astronomy and Astrophysics, Vol.275, NO. 1/AUG(I), P. 195, 1993

Astronomy and Astrophysics

Astrophysics

85

Stars: Formation, Interstellar Medium: Clouds

Scientific paper

Submillimetre and millimetre continuum observations of the Serpens star-forming cloud core have revealed six discrete objects, four of which have no near IR counterparts. We propose that these represent a second, more recent phase of star formation in the core. The strongest submm source corresponds to a known FIR and IRAS source-Serpens FIRS1, and shows an elongated lobe parallel to jet-like features seen at other wavelengths.

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