OH and the earliest evolution of H2 regions

Details OH and the earliest evolution of H2 regions OH and the earliest evolution of H2 regions

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hrgc.conf..127h&link_type=abstract

H II regions and the galactic centre : proceedings of the Eighth ESLAB Symposium, 4-7 June 1974, Frascati, Italy, p. 127-134 (SE

Astronomy and Astrophysics

Astronomy

1

Galactic Evolution, Hydrogen Clouds, Hydroxyl Emission, Masers, Radio Sources (Astronomy), Astronomical Maps, Continuous Radiation, Galactic Structure, Radio Emission, Radio Telescopes, Superhigh Frequencies, Ultrahigh Frequencies

Scientific paper

The continuum radiation near 13 type 1 OH masers, whose position was determined previously to within a few arc seconds, was mapped. Both ON1 and ON2 were included in the maser samples. The Westerbork Radio Telescope was used for this purpose at 6 and 21 cm. Isolated objects were also observed with the 100m Effelsberg (Bonn) telescope at 2.8 cm. It was found that compact H2 regions have a tendency to cluster on several scale sizes. The OH masers may coincide to within a few arc seconds with compact H2 regions. No OH masers were found to coincide with visible compact H2 regions such as K3-50.

Affiliated with

Also associated with

No associations

Rating

OH and the earliest evolution of H2 regions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with OH and the earliest evolution of H2 regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and OH and the earliest evolution of H2 regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1763990