Published April 10, 2010 | Version v1
Journal article

RXTE-BASED 35 DAY CYCLE TURN-ON TIMES FOR HERCULES X-1

  • 1. Department of Physics and Astronomy, University of Calgary, Calgary, AB T2N 1N4 (Canada)

Description

The 35 day X-ray cycle of Hercules X-1 (Her X-1) has been the subject of intense study since its discovery over 30 years ago. This work summarizes the results of determination of 35 day cycle turn-on (TO) times based on Rossi X-Ray Timing Explorer (RXTE)/All-Sky Monitor (ASM) observations of Her X-1. We apply a cross-correlation method to the entire (RXTE/ASM) Her X-1 database acquired between 1996 February 20 and 2009 December 18. We obtain new TO times for 147 cycles, 94 of which have well-determined times. The results reveal a uniform distribution of TO times with orbital phase. This does not support previous results that suggest TO times cluster around a specific orbital phase, such as 0.2 or 0.7. We also find 35 day cycle lengths ranging from 33.2 days to 36.7 days, and an average cycle length of 34.7 days.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/713/1/318

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
713
Journal Issue
1
Journal Page Range
p. 318-324
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41125966
Subject category
S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CORRELATIONS; DISTRIBUTION; NEUTRON STARS; NEUTRONS; X RADIATION
Descriptors DEC
BARYONS; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; HADRONS; IONIZING RADIATIONS; NUCLEONS; RADIATIONS; STARS