102-MHz observations of M33

Details 102-MHz observations of M33 102-MHz observations of M33

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..739a&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, Oct. 1986, p. 739-744) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, Sept.-Oc

Astronomy and Astrophysics

Astronomy

1

Astronomical Spectroscopy, Blue Stars, Local Group (Astronomy), Radio Sources (Astronomy), Spiral Galaxies, Supernova Remnants, Astronomical Maps, Disk Galaxies, Giant Stars, Radiant Flux Density, Spectral Resolution

Scientific paper

Interplanetary scintillation observations of M33 have been made at the frequency of 102 MHz. 17 scintillating sources have been observed in a 6°×4° region around the galaxy. No scintillating source has been found in M33 itself. A 102 MHz map of an area around M33 has been made with the resolution 49arcmin×29arcmin. The integral flux density at this frequency is S = 15±4 J. The supernova remnants density in M33 is one order of magnitude higher than in M31.

Affiliated with

Also associated with

No associations

Rating

102-MHz observations of M33 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 102-MHz observations of M33, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 102-MHz observations of M33 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1740365