Subarcsecond Resolution Observations of the G31.41+0.31 Hot Molecular Core

Details Subarcsecond Resolution Observations of the G31.41+0.31 Hot Molecular Core Subarcsecond Resolution Observations of the G31.41+0.31 Hot Molecular Core

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.2015h&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #20.15; Bulletin of the American Astronomical Society, Vol. 34, p.1136

Astronomy and Astrophysics

Astronomy

Scientific paper

In an effort to investigate the interior structure of Hot Molecular Cores we have imaged the G31.41+0.31 region at a wavelength of 7 mm with subarcsecond angular resolution. Our observations fully resolve the Hot Molecular Core and we detect an elongated structure, which we discuss in terms of an accretion disk scenario, as well as a binary scenario. This work is partially supported by Research Corporation grant Nr. CC4996 and NSF grant AST-0098524.

Affiliated with

Also associated with

No associations

Rating

Subarcsecond Resolution Observations of the G31.41+0.31 Hot Molecular Core 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 Subarcsecond Resolution Observations of the G31.41+0.31 Hot Molecular Core, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Subarcsecond Resolution Observations of the G31.41+0.31 Hot Molecular Core will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1889492