A Strong Flare of the H2O Maser in Sagittarius B2(M)

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Scientific paper

Results of a study of a strong flare of H2O maser emission in the star-forming region Sgr B2(M) in 2004 are reported. The observations were carried out on the 22-m radio telescope of the Pushchino Radio Astronomy Observatory. The main emission, with its flux density reaching 3800 Jy, was concentrated in a narrow radial-velocity interval (about 3 km/s) and was most likely associated with the compact group r, while the emission at V LSR > 64 km/s came from group q. After 1994, the variations of the H2O maser emission in Sgr B2(M) became cyclic with a mean period of 3 years.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

A Strong Flare of the H2O Maser in Sagittarius B2(M) 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 A Strong Flare of the H2O Maser in Sagittarius B2(M), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Strong Flare of the H2O Maser in Sagittarius B2(M) will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1620611

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.