Analysis of velocity components along the line of side towards SgrB2(M)

Details Analysis of velocity components along the line of side towards SgrB2(M) Analysis of velocity components along the line of side towards SgrB2(M)

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..280p.109b&link_type=abstract

The Molecular Universe, Posters from the proceedings of the 280th Symposium of the International Astronomical Union held in Tole

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the results of modeling the velocity components along the line of sight towards SgrB2(M) for different isotopologues of the molecules CO and CH+. The velocity components are a good tracer for the composition of the spiral arms of the Milky Way. The models were fit, with the programs myXCLASS and MAGIX, to the data of the interferometer Plateau de Bure and SMA, and the HEXOS KP data taken with the HIFI instrument aboard the Herschel Space Observatory. From the column densities of the isotopes one can determine the abundance ratios of the isotopologues as a function of velocity.

Affiliated with

Also associated with

No associations

Rating

Analysis of velocity components along the line of side towards SgrB2(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 Analysis of velocity components along the line of side towards SgrB2(M), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysis of velocity components along the line of side towards SgrB2(M) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-929229