An accurate position for the 6-cm OH masers in W3

Details An accurate position for the 6-cm OH masers in W3 An accurate position for the 6-cm OH masers in W3

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aj.....87.1806r&link_type=abstract

Astronomical Journal, vol. 87, Dec. 1982, p. 1806-1809.

Astronomy and Astrophysics

Astronomy

2

Hydroxyl Emission, Interstellar Masers, Accuracy, Ground State, H Ii Regions, Position (Location), Spectrophotometry

Scientific paper

The VLA has been used as a narrowband spectrophotometer to verify that the 6-cm emission from rotationally excited OH in W3OH is maser emission, and to measure its position. The 4765-MHz emission, like the ground-state emission, arises from gas in front of the compact H II region, apparently falling into it, and is not associated with the nearby H2O maser complex.

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