The optical pulsar H 2252-035 (AO Psc)

Details The optical pulsar H 2252-035 (AO Psc) The optical pulsar H 2252-035 (AO Psc)

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983msngr..34...33k&link_type=abstract

ESO Messenger (ISSN 0722-6691), Dec. 1983, p. 33-35.

Astronomy and Astrophysics

Astronomy

3

Astronomical Photometry, Binary Stars, Pulsars, Light Curve, Orbits, X Ray Sources

Scientific paper

The optical pulsar H2252-035 has been observed with a standard UBV photometer at La Silla Observatory, using an integration time of 5 sec in each bandpass. Attention is given to the results of a periodogram analysis of the data in which amplitudes are given in intensity units. These data, after subtraction of the short period modulations, were folded with the orbital period to yield average light and color curves. It appears that the site at which the original radiation is being reprocesed is located far enough from the disk so that both illuminating and reprocessed radiations can travel to and from it relatively undisturbed. The stability of the 859- and 805-sec periods is noted.

Affiliated with

Also associated with

No associations

Rating

The optical pulsar H 2252-035 (AO Psc) 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 The optical pulsar H 2252-035 (AO Psc), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The optical pulsar H 2252-035 (AO Psc) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1805257