Neon Line Emission in the X-Ray Spectrum of the Pulsar 4U 1626−67-Reference-Cited by-同舟云学术

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Neon Line Emission in the X-Ray Spectrum of the Pulsar 4U 1626−67

Published:1995-08-10 Issue:1 Volume:449 Page:
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Angelini L.,White N. E.,Nagase F.,Kallman T. R.,Yoshida A.,Takeshima T.,Becker C.,Paerels F.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference28 articles.

1. Abundances of the elements: Meteoritic and solar

2. Angelini, L., Ghosh, P. & White, N. E. 1994, in New Horizon of X-Ray Astronomy-First Results from ASCA, ed. F. Makino & T. Ohashi (Tokyo: Universal Academy Press), 411

3. Hydrostatic nucleosynthesis. I - Core helium and carbon burning.

Cited by 66 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. The ongoing spin-down episode of 4U 1626-67;Monthly Notices of the Royal Astronomical Society;2024-01-23

2. UltraCompCAT: A comprehensive catalogue of ultra-compact and short orbital period X-ray binaries;Astronomy & Astrophysics;2023-09

3. 4U 1626−67 returns to spin-down: timing features toe the line;Monthly Notices of the Royal Astronomical Society: Letters;2023-08-04

4. Observations of 4U 1626–67 with the Imaging X-Ray Polarimetry Explorer;The Astrophysical Journal;2022-11-01

5. Chandra/LETGS Studies of the Collisional Plasma in 4U 1626–67;The Astrophysical Journal;2021-10-01

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