PHYSICAL STRUCTURE OF THE PLANETARY NEBULA NGC 3242 FROM THE HOT BUBBLE TO THE NEBULAR ENVELOPE-Reference-Cited by-同舟云学术

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PHYSICAL STRUCTURE OF THE PLANETARY NEBULA NGC 3242 FROM THE HOT BUBBLE TO THE NEBULAR ENVELOPE

Published:2011-08-16 Issue:3 Volume:142 Page:91
ISSN:0004-6256
Container-title:The Astronomical Journal
language:
Short-container-title:The Astronomical Journal

Author:

Ruiz Nieves,Guerrero Martín A.,Chu You-Hua,Gruendl Robert A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference41 articles.

1. FLIERs and Other Microstructures in Planetary Nebulae. IV. Images of Elliptical PNs from the [ITAL]Hubble[/ITAL] [ITAL]Space[/ITAL] [ITAL]T[/ITAL][ITAL]elescope[/ITAL]

2. The evolution of planetary nebulae. II - Dynamical evolution of elliptical PNs and collimated outflows

3. Fast, low-ionization emission regions and other microstructures in planetary nebulae

4. Winds in central stars of planetary nebulae

5. [ITAL]Chandra[/ITAL] Reveals the X-Ray Glint in the Cat’s Eye

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2. The X-ray Emission from Planetary Nebulae;Handbook of X-ray and Gamma-ray Astrophysics;2024

3. The X-Ray Emission from Planetary Nebulae;Handbook of X-ray and Gamma-ray Astrophysics;2022-09-23

4. X-ray Observations of Planetary Nebulae since WORKPLANS I and Beyond;Galaxies;2020-03-17

5. Understanding nebular spectra of Type Ia supernovae;Monthly Notices of the Royal Astronomical Society;2020-03-09

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