Short-term variations in Class I methanol masers?

Details Short-term variations in Class I methanol masers? Short-term variations in Class I methanol masers?

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..242...34p&link_type=abstract

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

Astronomy and Astrophysics

Astrophysics

1

Masers, Stars:Formation

Scientific paper

Class I methanol masers are found near regions of high-mass star formation and are pumped by collisions. Some indication of long-term variability in these masers has previously been reported (Kurtz et al. 2004). Here we will present evidence for variations in the intensity of the Class I methanol masers at 44 GHz on much shorter timescales. We present preliminary results of the observation of the 44 GHz Class I methanol transition toward sources in the DR21 region that indicates variability on timescales of days to possibly hours.

Affiliated with

Also associated with

No associations

Rating

Short-term variations in Class I methanol masers? 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 Short-term variations in Class I methanol masers?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Short-term variations in Class I methanol masers? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-862624