Detection of Photodissociated Gas Toward the HII Region GGD12-15

Details Detection of Photodissociated Gas Toward the HII Region GGD12-15 Detection of Photodissociated Gas Toward the HII Region GGD12-15

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001rmxac..11...69g&link_type=abstract

"IX Latin American Regional IAU Meeting, "Focal Points in Latin American Astronomy", held in Tonantzintla, Mexico, Nov 9-13, 199

Astronomy and Astrophysics

Astronomy

Scientific paper

We present VLA continuum (2, 3.6 and 20 cm) and line (H~I 21 cm, H92α and C92α) observations toward the cometary-like H~II region near the optical nebulosities GGD~12--15. The hydrogen recombination line (RRL) observations show that the ionized gas is undergoing a champagne flow. The carbon RRL and the 21~cm emission detected toward the H~II region have line center velocities similar to the velocity of the ambient molecular cloud. Both the carbon RRL and H~I emissions are interpreted as arising from the photodissociated gas around the H~II region. Using an isothermal model for photodissociated regions (PDRs) we estimate the physical parameters of this region.

Affiliated with

Also associated with

No associations

Rating

Detection of Photodissociated Gas Toward the HII Region GGD12-15 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 Detection of Photodissociated Gas Toward the HII Region GGD12-15, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of Photodissociated Gas Toward the HII Region GGD12-15 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1206028