Aperture synthesis maps of HDO emission in Orion-KL

Details Aperture synthesis maps of HDO emission in Orion-KL Aperture synthesis maps of HDO emission in Orion-KL

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...317l.101p&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 317, June 15, 1987, p. L101-L105.

Astronomy and Astrophysics

Astrophysics

67

Astronomical Maps, Heavy Water, Interstellar Gas, Orion Nebula, Abundance, Nebulae, Synthetic Apertures

Scientific paper

The 110-111 transition of deuterated water has been mapped toward the Kleinmann-Low nebula in Orion with the Hat Creek millimeter interferometer. The synthesized beamwidth is 3arcsec.4. The "hot core", "plateau", and "compact ridge" emission regions can be identified on the maps. The compact ridge appears to consist of streamers of gas which connect to the hot core clump and are directed away from the source IRc 2. The HDO/H2 abundance toward both hot core and compact ridge is inferred to be ≡10-7, unexpectedly high for such warm regions.

Affiliated with

Also associated with

No associations

Rating

Aperture synthesis maps of HDO emission in Orion-KL 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 Aperture synthesis maps of HDO emission in Orion-KL, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Aperture synthesis maps of HDO emission in Orion-KL will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1814193