Improved () 3He Abundances in HII Regions

Details Improved () 3He Abundances in HII Regions Improved () 3He Abundances in HII Regions

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...183.9203b&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #92.03; Bulletin of the American Astronomical Society, Vol. 25, p.1433

Astronomy and Astrophysics

Astronomy

Scientific paper

Numerical models have been developed to improve the (3) He measurements discussed by Bania et al. at this meeting. A triad of observations have been used to constrain these models. Continuum ``snapshots'' have been taken with the VLA in D-array at X band to provide information at a high angular resolution. The MPIfR 100 m telescope has also been used to map the extended continuum emission of these regions. Lastly, as a byproduct of the NRAO 43 m (3) He(+) observations, many radio recombination lines have been simultaneously measured. These observations provide information about the electron temperature and small-scale density clumping. This ongoing work should yield (3) He abundances with an accuracy of 10% for some sources. The implications of these results are reported by Rood et al. at this meeting.

Affiliated with

Also associated with

No associations

Rating

Improved () 3He Abundances in HII Regions 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 Improved () 3He Abundances in HII Regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Improved () 3He Abundances in HII Regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-780830