H2O maser emission from HH 6 and other star-forming regions

Details H2O maser emission from HH 6 and other star-forming regions H2O maser emission from HH 6 and other star-forming regions

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...165..197h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 165, no. 1-2, Sept. 1986, p. 197-203.

Astronomy and Astrophysics

Astrophysics

56

Interstellar Masers, Molecular Clouds, Star Formation, Water Masers, Data Correlation, Galactic Structure, H Ii Regions, Herbig-Haro Objects, Traveling Waves

Scientific paper

A search for water vapor maser emission toward the S 254-257 region, toward prominent outflow sources, and toward H II regions and giant molecular clouds in the outer galaxy is presented. Four new masers are found: toward S 255, S 256, GL 490, and HH 6. The maser in HH 6 coincides in position (within 1 arcsec) with a compact radio continuum source, which might contain the exciting source of the HH region. In S 76 E and S 87, two spatially separated components are detected. Toward the outer galaxy, negative results are reported in 11 Sharpless regions and five giant molecular clouds.

Affiliated with

Also associated with

No associations

Rating

H2O maser emission from HH 6 and other star-forming 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 H2O maser emission from HH 6 and other star-forming regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and H2O maser emission from HH 6 and other star-forming regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1290024