A search for H2O maser emission in the Serpens region

Details A search for H2O maser emission in the Serpens region A search for H2O maser emission in the Serpens region

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...223..267p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 223, no. 1-2, Oct. 1989, p. 267-270.

Astronomy and Astrophysics

Astronomy

6

Infrared Sources (Astronomy), Interstellar Masers, Molecular Clouds, Pre-Main Sequence Stars, Water Masers, Far Infrared Radiation, Luminosity, T Tauri Stars, Water Vapor

Scientific paper

This paper presents the results of repeated H2O maser line observations (22.2 GHz) in the Serpens region obtained with the 32-m parabola of the Medicina Station over a period of 16 months. Several positions coincident with pre-main-sequence objects and far-infrared sources were observed, with no positive detection at an average rms = 1.5 Jy. In addition, three regions were mapped: the cloud molecular core, the Ser/G3-G6 complex, and the strong IRAS source 18278+O111. Only within the core, and only in one out of six observing runs, a feature of 48 Jy was observed. This line coincides in position and velocity with one of the two masers reported by Blair et al. (1975), but never detected since then.

Affiliated with

Also associated with

No associations

Rating

A search for H2O maser emission in the Serpens region 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 A search for H2O maser emission in the Serpens region, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A search for H2O maser emission in the Serpens region will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1526995