On the relationship between the infrared source CRL 2591 /UOA-27/ and its radio and H2O counterparts

Details On the relationship between the infrared source CRL 2591 /UOA-27/ and its radio and H2O counterparts On the relationship between the infrared source CRL 2591 /UOA-27/ and its radio and H2O counterparts

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...211l..89w&link_type=abstract

Astrophysical Journal, vol. 211, Jan. 15, 1977, pt. 2, p. L89, L90.

Astronomy and Astrophysics

Astronomy

48

Infrared Radiation, Radio Sources (Astronomy), Stellar Evolution, Water Masers, Angular Resolution, Astronomical Photometry, H Ii Regions, Interstellar Masers, Nebulae, Protostars

Scientific paper

Recent radio, infrared, and H2O maser observations show that there is a 7-arcsec angular separation between the protostarlike infrared source CRL 2591 and the compact H II region which has until now been identified with it, while the H2O maser coincides with the infrared source. This result, together with an extension of photometric measurements to 20 microns and a much improved upper limit to its angular size, reinforces the apparent similarity of CRL 2591 to the BN object in Orion and to W3/IRS 5.

Affiliated with

Also associated with

No associations

Rating

On the relationship between the infrared source CRL 2591 /UOA-27/ and its radio and H2O counterparts 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 On the relationship between the infrared source CRL 2591 /UOA-27/ and its radio and H2O counterparts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the relationship between the infrared source CRL 2591 /UOA-27/ and its radio and H2O counterparts will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-951755