Molecular hydrogen emission in HH complexes. I - AS 353A/HH 32

Details Molecular hydrogen emission in HH complexes. I - AS 353A/HH 32 Molecular hydrogen emission in HH complexes. I - AS 353A/HH 32

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...158l...9z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 158, no. 1-2, April 1986, p. L9-L11. Research supported by the Academy of Finl

Astronomy and Astrophysics

Astronomy

11

Emission Spectra, Herbig-Haro Objects, Hydrogen, Infrared Astronomy, Pre-Main Sequence Stars, Stellar Winds, High Resolution, Shock Waves, Spectrum Analysis, T Tauri Stars

Scientific paper

High resolution mapping (5 arc sec) of the bipolar outflow region AS 353A and HH 32A,B,C in the υ = 1-0 S(1) line of H2 shows that the shock excited H2 emission is closely associated with the visible Herbig-Haro objects. The authors find strong H2 emission centred on HH 32A and B and some evidence for emission toward HH 32C. They also find a faint bridge of emission extending from AS 353A to HH 32A,B, which has a visible counterpart on high contrast CCD images.

Affiliated with

Also associated with

No associations

Rating

Molecular hydrogen emission in HH complexes. I - AS 353A/HH 32 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 Molecular hydrogen emission in HH complexes. I - AS 353A/HH 32, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Molecular hydrogen emission in HH complexes. I - AS 353A/HH 32 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1101149