Structure of the source W3(OH) at 18-cm wavelength

Details Structure of the source W3(OH) at 18-cm wavelength Structure of the source W3(OH) at 18-cm wavelength

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..501a&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, June 1989, p. 501-507. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Circular Polarization, Interstellar Masers, Microwave Emission, Radio Sources (Astronomy), Brightness Distribution, Centimeter Waves, Normal Density Functions, Radio Interferometers

Scientific paper

The maser source W3(OH) was observed on December 1987 with the
Simeiz-Pushchino radio interferometer at frequencies of 1665 and 1667
MHz in left and right circulation polarization. The component sizes are
estimated under the assumption of a Gaussian brightness distribution,
and the distances between the components are determined.

Affiliated with

Also associated with

No associations

Rating

Structure of the source W3(OH) at 18-cm wavelength 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 Structure of the source W3(OH) at 18-cm wavelength, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure of the source W3(OH) at 18-cm wavelength will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1856388