The stability of the pulse intensity of the X-ray pulsar in the Crab Nebula

Details The stability of the pulse intensity of the X-ray pulsar in the Crab Nebula The stability of the pulse intensity of the X-ray pulsar in the Crab Nebula

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...103..367m&link_type=abstract

Astronomy and Astrophysics, vol. 103, no. 2, Nov. 1981, p. 367-369. Navy-supported research.

Astronomy and Astrophysics

Astronomy

Crab Nebula, Pulsars, Pulse Rate, Statistical Analysis, X Ray Astronomy, Heao 1, Light Curve, Periodic Variations, Radio Emission, Random Variables

Scientific paper

The large area detector on the H.E.A.O.-A satellite and the fast time
resolution, permitted us to detect individual Crab pulses. A statistical
analysis performed on those pulses shows, that although there are
pulse-to-pulse variations, they fall within the random expectation.

Affiliated with

Also associated with

No associations

Rating

The stability of the pulse intensity of the X-ray pulsar in the Crab Nebula 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 stability of the pulse intensity of the X-ray pulsar in the Crab Nebula, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The stability of the pulse intensity of the X-ray pulsar in the Crab Nebula will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-743312