X-ray emission by a shocked fast wind from the central stars of planetary nebulae
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/368/4/1706/3969949/mnras0368-1706.pdf
Reference23 articles.
1. Shapes and Shaping of Planetary Nebulae
2. Self-similar solutions for the interaction regions of colliding winds
3. High‐Resolution X‐Ray Image of the Hydrogen‐deficient Planetary Nebula Abell 30
4. [ITAL]Chandra[/ITAL] Reveals the X-Ray Glint in the Cat’s Eye
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1. Three scenarios for shaping ‘ears’ in planetary nebulae;New Astronomy;2023-01
2. THECHANDRAX-RAY SURVEY OF PLANETARY NEBULAE (CHANPLANS): PROBING BINARITY, MAGNETIC FIELDS, AND WIND COLLISIONS;The Astronomical Journal;2012-07-12
3. COMPARING SHOCKS IN PLANETARY NEBULAE WITH THE SOLAR WIND TERMINATION SHOCK;The Astrophysical Journal;2010-12-02
4. Diffuse X-ray emissions from dynamic planetary nebulae;Monthly Notices of the Royal Astronomical Society;2010-07-23
5. NARROW RADIATIVE RECOMBINATION CONTINUA: A SIGNATURE OF IONS CROSSING THE CONTACT DISCONTINUITY OF ASTROPHYSICAL SHOCKS;The Astrophysical Journal;2009-04-03
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