NH3 and H2O in the S106 molecular cloud

Details NH3 and H2O in the S106 molecular cloud NH3 and H2O in the S106 molecular cloud

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...111..201s&link_type=abstract

Astronomy and Astrophysics, vol. 111, no. 1, July 1982, p. 201-208. Deutsche Forschungsgemeinschaft

Astronomy and Astrophysics

Astrophysics

48

Ammonia, Astronomical Maps, Molecular Clouds, Molecular Spectra, Nebulae, Water Masers, Angular Resolution, Brightness Temperature, Nuclear Quadrupole Resonance, Point Sources

Scientific paper

The Effelsberg 100m telescope was used to simultaneously map the NH3 (J,K) equals (1,1) and (2,2) lines with an angular resolution of 40 arcsec in the molecular cloud surrounding the 'bipolar nebula' S106. The NH3 cloud consists of two parts located east and west of the visible nebula. There is no indication that the cloud forms a rotating ring. The intensities of the NH3 (1,1) nuclear quadrupole HfS components show strong deviations from LTE, which are position dependent. The H2O maser reported by Cesarsky et al. (1978) was not found; instead a new maser 13 arcsec west of the central IR-point source was detected.

Affiliated with

Also associated with

No associations

Rating

NH3 and H2O in the S106 molecular cloud 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 NH3 and H2O in the S106 molecular cloud, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and NH3 and H2O in the S106 molecular cloud will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1022046