Physical Conditions in HH39

Details Physical Conditions in HH39 Physical Conditions in HH39

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.2107i&link_type=abstract

American Astronomical Society, 187th AAS Meeting, #21.07; Bulletin of the American Astronomical Society, Vol. 27, p.1318

Astronomy and Astrophysics

Astronomy

Scientific paper

Physical conditions in the HH39 object are analysed using images taken in the light of Hα , [SII]lambda 6716 Angstroms, [SII]lambda 6731 Angstroms, and [NII]lambda 6584 Angstroms. Two-dimensional maps of the [SII]{lambda 6731}/{lambda 6716} ratio, resultant electron density, and the excitation - dependent ratios [SII]{lambda lambda 6716+6731}/H alpha , and [NII]lambda 6584/H alpha are calculated. Trends across the object place limitations on bow-shock and jet models of the object. A wide-field search for further shock activity in the R Monocerotis region, using images in the light of Hα and [SII]lambda lambda 6716+ 6731, shows that HH39 is isolated and probably not part of a larger flow.

Affiliated with

Also associated with

No associations

Rating

Physical Conditions in HH39 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 Physical Conditions in HH39, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physical Conditions in HH39 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1253290