SPECTRAL AND TIMING NATURE OF THE SYMBIOTIC X-RAY BINARY 4U 1954+319: THE SLOWEST ROTATING NEUTRON STAR IN AN X-RAY BINARY SYSTEM-Reference-Cited by-同舟云学术

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SPECTRAL AND TIMING NATURE OF THE SYMBIOTIC X-RAY BINARY 4U 1954+319: THE SLOWEST ROTATING NEUTRON STAR IN AN X-RAY BINARY SYSTEM

Published:2014-04-24 Issue:2 Volume:786 Page:127
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Enoto Teruaki,Sasano Makoto,Yamada Shin'ya,Tamagawa Toru,Makishima Kazuo,Pottschmidt Katja,Marcu Diana,Corbet Robin H. D.,Fuerst Felix,Wilms Jörn

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/786/i=2/a=127/pdf

Reference91 articles.

1. The Chemical Composition of the Sun

2. Photoelectric absorption cross sections with variable abundances

3. A description of sources detected by INTEGRAL during the first 4 years of observations

4. CHANDRAOBSERVATIONS OF FIVEINTEGRALSOURCES: NEW X-RAY POSITIONS FOR IGR J16393–4643 AND IGR J17091–3624

5. Are There Magnetars in High‐Mass X‐Ray Binaries? The Case of Supergiant Fast X‐Ray Transients

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1. On the ultra-long spin period of 4U 1954+31;Monthly Notices of the Royal Astronomical Society;2024-07-24

2. On Its Way to the Neutron Star–White Dwarf Binary Graveyard, IGR J16194−2810, A First Ascent M Giant X-Ray Binary;The Astrophysical Journal;2024-07-01

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4. Peering into the central region of a nano-quasar: XMM–Newton and Chandra views of the CH Cyg symbiotic system;Monthly Notices of the Royal Astronomical Society;2023-05-10

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