Search for optical emission from radio pulsars on the six-meter telescope

Details Search for optical emission from radio pulsars on the six-meter telescope Search for optical emission from radio pulsars on the six-meter telescope

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..742l&link_type=abstract

(Astronomicheskii Zhurnal, vol. 60, July-Aug. 1983, p. 742-745) Soviet Astronomy (ISSN 0038-5301), vol. 27, July-Aug. 1983, p. 4

Astronomy and Astrophysics

Astronomy

Light Emission, Pulsars, Radio Sources (Astronomy), Astronomical Catalogs, Luminous Intensity, Stellar Magnitude

Scientific paper

Upper limits on visible emissions are determined for the radio pulsars 0105+65, 0301+19, 0329+54, 0450-18, 0611+22, 0655+64, 0919+06, and 1915+13 on the basis of 30-min photometric observations obtained with the 6-m telescope at the USSR Special Astrophysical Observatory during 1980-1981. The B-band limits are calculated by assuming a spectrum like that of the Crab Nebula pulsar (0531+21) and presented in a table. The respective limits are 25.1, 24.9, 26.9, 25.6, 26.9, 24.6, and 26.5 mag.

Affiliated with

Also associated with

No associations

Rating

Search for optical emission from radio pulsars on the six-meter telescope 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 Search for optical emission from radio pulsars on the six-meter telescope, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Search for optical emission from radio pulsars on the six-meter telescope will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-741912