Radio Molecular lines in infrared dark clouds (Ragan+, 2006)

Details Radio Molecular lines in infrared dark clouds (Ragan+, 2006) Radio Molecular lines in infrared dark clouds (Ragan+, 2006)

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..21660567r&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/166/567. Originally published in: 2006ApJS..166..567R

Astronomy and Astrophysics

Astronomy

Scientific paper

We mapped 41 of the sample of MSX dark clouds in emission from C18 J=1->0 (nu=109.782GHz), CS J=2->1 (nu=97.981GHz), and N2H+ J=1->0 (nu=93.173GHz) using the 14m Five College Radio Astronomy Observatory (FCRAO). The observations were made in 2002 February, May, and December using the 16 element focal plane array receiver SEQUOIA.
(3 data files).

Affiliated with

Also associated with

No associations

Rating

Radio Molecular lines in infrared dark clouds (Ragan+, 2006) 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 Radio Molecular lines in infrared dark clouds (Ragan+, 2006), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio Molecular lines in infrared dark clouds (Ragan+, 2006) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1077605