An Analysis of the Dust Halo and Extinction toward X Persei

Author:

Valencic Lynne A.,Smith Randall K.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference93 articles.

1. Anders, E. & Grevesse, N. 1989, Geochim. Cosmochim. Acta, 53, 197 (AG89)

2. Asplund, M., Sauval, J. & Grevesse, N. 2005, in ASP Conf. Ser. 336, Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, ed. T. G. Barnes, III, & F. N. Bash (San Francisco: ASP), 25 (ASG05)

3. Physical conditions in the Orion Nebula and an assessment of its helium abundance

4. The nature of the X-ray halo of the plerion G21.5–0.9 unveiled by XMM-Newton and Chandra

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1. Effects of Interstellar Dust Scattering on the X-ray Eclipses of the LMXB AX J1745.6-2901 in the Galactic Center;Monthly Notices of the Royal Astronomical Society;2018-04-06

2. Probing the interstellar dust towards the Galactic Centre: dust-scattering halo around AX J1745.6−2901;Monthly Notices of the Royal Astronomical Society;2017-03-16

3. The dust scattering halo of Cygnus X-3;Monthly Notices of the Royal Astronomical Society;2015-08-24

4. INTERSTELLAR ABUNDANCES TOWARD X Per, REVISITED;The Astrophysical Journal;2013-05-20

5. AZIMUTHAL STRUCTURE OF THE Cyg X-2 X-RAY DUST HALO;The Astrophysical Journal;2013-04-30

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