A MULTI-WAVELENGTH 3D MODEL OF BD+30°3639
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/0067-0049/226/2/15/pdf
Reference66 articles.
1. X-ray emission from jet–wind interaction in planetary nebulae
2. ‘Distance mapping’ and the 3D structure of BD +30° 3639
3. X-Ray Emission from the Wind-Blown Bubble in the Planetary Nebula BD +30°3639
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1. Hot bubbles of planetary nebulae with hydrogen-deficient winds;Astronomy & Astrophysics;2024-04
2. Discovery of Radial Spectral Hardening in the Hot Bubble of Planetary Nebula BD+30°3639 with Median Energy Imaging;The Astrophysical Journal;2024-03-01
3. FAST Search for Circumstellar Atomic Hydrogen. II. Is BD+30°3639 an Interacting Planetary Nebula?;The Astrophysical Journal;2023-07-27
4. Dissociative single and double photoionization of biphenyl (C12H10) by soft X-rays in planetary nebulae;Monthly Notices of the Royal Astronomical Society;2020-10-15
5. X-ray Observations of Planetary Nebulae since WORKPLANS I and Beyond;Galaxies;2020-03-17
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