Water maser flares in W75N

Details Water maser flares in W75N Water maser flares in W75N

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..737l&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Oct. 1984, p. 737-740) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Sept.-Oc

Astronomy and Astrophysics

Astronomy

2

Hydrogen Clouds, Interstellar Masers, Radio Sources (Astronomy), Water Masers, Bursts, Line Spectra, Long Term Effects, Radiant Flux Density

Scientific paper

The results of radio observations of the water maser flares of the H II (B) region of the W75N star nursery are reported. The scans were performed from 1981-1983, which allowed acquisition of data during the declining phases of two flare events. Also observed during one 7-month period was a continuous flux intensity accompanied by a slow drift in the line profile. Interferometric measurements limited the maser source to a region no more than 10 to the 17th cm across. It is suggested that the pumping source must be radiative if the region scanned is one of star formation.

Affiliated with

Also associated with

No associations

Rating

Water maser flares in W75N 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 Water maser flares in W75N, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Water maser flares in W75N will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1229870