Brightness Distributions of Radio Sources at 2-Centimeter Wavelength

Details Brightness Distributions of Radio Sources at 2-Centimeter Wavelength Brightness Distributions of Radio Sources at 2-Centimeter Wavelength

Sep 1966

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1966sci...153.1107z&link_type=abstract

Science, Volume 153, Issue 3740, pp. 1107-1109

Physics

15

Scientific paper

Maps have been made of the 2-centimeter brightness distribution of M17, Cassiopeia-A, Taurus-A, and Orion nebula with a resolution of 2.3 minutes of arc, revealing several newly resolved features. M17 is a double thermal source. Some structure appears in Cassiopeia-A, including a suggestion of a ring shape. Taurus-A exhibits a brightness map similar to that obtained in earlier low-frequency results. The central part of Orion nebula is circularly symmetric to a high degree of accuracy.

Affiliated with

Also associated with

No associations

Rating

Brightness Distributions of Radio Sources at 2-Centimeter 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 Brightness Distributions of Radio Sources at 2-Centimeter Wavelength, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Brightness Distributions of Radio Sources at 2-Centimeter Wavelength will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1241465