Universal detection of high-temperature emission in X-ray isolated neutron stars-Reference-Cited by-同舟云学术

Universal detection of high-temperature emission in X-ray isolated neutron stars

Published:2019-01-01 Issue:1 Volume:71 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Yoneyama Tomokage¹²,Hayashida Kiyoshi¹²,Nakajima Hiroshi³,Matsumoto Hironori¹²

Affiliation:

1. Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama-cho, Toyonaka, Osaka 560-0043, Japan

2. Project Research Center for Fundamental Sciences, Graduate School of Science, Osaka University, 1-1 Machikaneyama-cho, Toyonaka, Osaka 560-0043, Japan

3. College of Science and Engineering, Kanto Gakuin University, 1-50-1 Mutsuurahigashi, Kanazawa-ku, Yokohama, Kanagawa 236-8501, Japan

Funder

Japan Society for the Promotion of Science

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/71/1/17/27641488/psy135.pdf

Reference47 articles.

1. Establishing HZ43 A, Sirius B, and RX J185635-3754 as soft X-ray standards: a cross-calibration between the Chandra LETG+HRC-S, the EUVE spectrometer, and the ROSAT PSPC

2. DISCOVERY OF A STRONGLY PHASE-VARIABLE SPECTRAL FEATURE IN THE ISOLATED NEUTRON STAR RX J0720.4–3125

3. Narrow phase-dependent features in X-ray dim isolated neutron stars: a new detection and upper limits

4. Phase-Resolved Spectroscopy of Geminga Shows Rotating Hot Spot(s)

5. Maximum gravitational-wave energy emissible in magnetar flares

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