OB star formation in the S128 region

Details OB star formation in the S128 region OB star formation in the S128 region

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...243..526h&link_type=abstract

Astrophysical Journal, Part 1, vol. 243, Jan. 15, 1981, p. 526-532. Research supported by the University of California

Astronomy and Astrophysics

Astronomy

20

B Stars, Interstellar Masers, O Stars, Star Formation, Water Masers, Astronomical Maps, H Ii Regions, Radio Astronomy, Very Large Array (Vla)

Scientific paper

The H II region S128 was mapped using the Very Large Array and the Westerbork Synthesis Radio Telescope at 6 and 20 cm wavelengths. A compact (approximately 3 arcsec) H II region was observed approximately 60 arcsec north of the more extended H II region whose radio structure corresponds to the optical emission. An H2O maser source was detected offset from the compact source by approximately 12 arcsec. This indicates three separate sites of star formation in this region. Various schemes of initiating star formation are discussed with reference to this distant H II region.

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