An OH maser flare with a strong magnetic field in W75N

Details An OH maser flare with a strong magnetic field in W75N An OH maser flare with a strong magnetic field in W75N

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..242..166s&link_type=abstract

Astrophysical Masers and their Environments, Proceedings of the International Astronomical Union, IAU Symposium, Volume 242, p.

Astronomy and Astrophysics

Astrophysics

Ism:Magnetic Fields, Stars: Flare, Maser

Scientific paper

A flare of OH maser emission was discovered in W75N in 2000. Its location was determined with the VLBA to be within 110 AU from one of the ultra-compact HII regions, VLA2. The flare consisted of several maser spots. Four of the spots were found to form Zeeman pairs, all of them with a magnetic field strength of about 40 mG. This is the highest ever magnetic field strength found in OH masers, an order of magnitude higher than in typical OH masers. We discuss the possible source for the enhanced magnetic field and its relation to the flare event.

Affiliated with

Also associated with

No associations

Rating

An OH maser flare with a strong magnetic field 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 An OH maser flare with a strong magnetic field in W75N, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An OH maser flare with a strong magnetic field in W75N will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-922633