The nature of the Stingray nebula from radio observations-Reference-Cited by-同舟云学术

The nature of the Stingray nebula from radio observations

Published:2018-06-11 Issue:2 Volume:479 Page:1842-1849
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Harvey-Smith Lisa¹²³^ORCID,Hardwick Jennifer A¹,De Marco Orsola⁴,Parthasarathy Mudumba⁵,Gonidakis Ioannis¹,Akhter Shaila¹²,Cunningham Maria²,Green James A¹

Affiliation:

1. CSIRO Astronomy and Space Science, Australia Telescope National Facility, PO Box 76, Epping 1710, Australia

2. School of Physics, University of New South Wales, NSW 2052, Australia

3. Western Sydney University, Locked Bag 1797, Penrith, NSW 2751, Australia

4. Department of Physics, Macquarie University, Sydney NSW 2109, Australia

5. Indian Institute of Astrophysics, Bangalore 560034, India

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/479/2/1842/25135143/sty1513.pdf

Reference29 articles.

1. High-resolution radio continuum observations of compact planetary nebulae

2. Rapid photometric and spectroscopic evolution of the young planetary nebula Hen 3–1357 and its central star SAO 244567

3. Birth and early evolution of a planetary nebula

4. The Stingray Nebula: watching the rapid evolution of a newly born planetary nebula

5. Radio variability and non-thermal components in stars evolving towards planetary nebulae

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1. Evolution of Hen 3-1357, the Stingray Nebula;Monthly Notices of the Royal Astronomical Society;2022-06-24

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4. The Decline and Fall of the Youngest Planetary Nebula;The Astrophysical Journal;2021-02-03