Space Telescope Imaging Spectrograph Ultraviolet Spectra of Large Magellanic Cloud Planetary Nebulae: A Study of Carbon Abundances and Stellar Evolution-Reference-Cited by-同舟云学术

Space Telescope Imaging Spectrograph Ultraviolet Spectra of Large Magellanic Cloud Planetary Nebulae: A Study of Carbon Abundances and Stellar Evolution

Published:2005-03-20 Issue:1 Volume:622 Page:294-318
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Stanghellini Letizia,Shaw Richard A.,Gilmore Diane

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/622/i=1/a=294/pdf

Reference41 articles.

1. Aller, L. H. 1984, Physics of Thermal Gaseous Nebulae (Dordrecht: Reidel)

2. The relationship between infrared, optical, and ultraviolet extinction

3. Cox, A. N. 2000, Allen’s Astrophysical Quantities (4th ed.; New York: AIP)

4. Hubble Space Telescope Observations of Planetary Nebulae in the Magellanic Clouds. IV. [O iii] Images and Evolutionary Ages

5. Feibelman, W. A., Oliversen, N. A., Nicholsbohlin, J. & Garhart, M. P. 1988, International Ultraviolet Explorer Spectral Atlas of Planetary Nebulae, Central Stars, and Related Objects (Washington: NASA)

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