Probing the Birth of Hot Cores through Mid-Infrared and Submillimeter Spectroscopy of HCN and C2H2

Details Probing the Birth of Hot Cores through Mid-Infrared and Submillimeter Spectroscopy of HCN and C2H2 Probing the Birth of Hot Cores through Mid-Infrared and Submillimeter Spectroscopy of HCN and C2H2

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..267..345b&link_type=abstract

Hot Star Workshop III: The Earliest Stages of Massive Star Birth. ASP Conference Proceedings, Vol. 267. Edited by Paul A. Crowth

Astronomy and Astrophysics

Astronomy

Scientific paper

High-resolution spectroscopy in the infrared and submillimeter shows
that the hot gas in massive protostars is located in the inner envelope
and can be used to probe the birth of hot cores.

Affiliated with

Also associated with

No associations

Rating

Probing the Birth of Hot Cores through Mid-Infrared and Submillimeter Spectroscopy of HCN and C2H2 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 Probing the Birth of Hot Cores through Mid-Infrared and Submillimeter Spectroscopy of HCN and C2H2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Probing the Birth of Hot Cores through Mid-Infrared and Submillimeter Spectroscopy of HCN and C2H2 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1661514