The Distribution of the 2PI3/2J = 3/2OH Maser Emission Associated with W49N

Details The Distribution of the 2PI3/2J = 3/2OH Maser Emission Associated with W49N The Distribution of the 2PI3/2J = 3/2OH Maser Emission Associated with W49N

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aj.....87..803j&link_type=abstract

ASTRONOMICAL JOURNAL V. 87, P. 803, 1982

Astronomy and Astrophysics

Astronomy

11

Scientific paper

The OH emission in the 2π3/2J =3/2 F = 1→1 and F = 2→2 transitions associated with W49N was found to lie in an area 10" × 8". The radiation appears to surround the intense H2O masers and the compact continuum source. The majority of the spectral features which lie between 10 and 20 km s are clumped in an area of diameter less than 1". The features between -2 and +7 km s-1 may be caused by an outflow of material from the continuum position, while the features between 10 and 20 km s-1 are probably associated with mass outflow from a compact object located at their position.

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