The kinematic behaviour of optical recombination lines and collisionally excited lines in Galactic planetary nebulae*†-Reference-Cited by-同舟云学术

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The kinematic behaviour of optical recombination lines and collisionally excited lines in Galactic planetary nebulae*†

Published:2017-09-09 Issue:1 Volume:472 Page:1182-1194
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Peña Miriam¹,Ruiz-Escobedo Francisco¹,Rechy-García Jackeline S.¹,García-Rojas Jorge²³

Affiliation:

1. Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 70264, Cd. de México, 04510, México

2. Instituto de Astrofísica de Canarias (IAC), E-38200 La Laguna, Tenerife, Spain

3. Universidad de La Laguna, Department Astrofísica. E-38206 La Laguna, Tenerife, Spain

Funder

MINECO

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/472/1/1182/19730144/stx1991.pdf

Reference46 articles.

1. Quantitative classification of WR nuclei of planetary nebulae

2. The Spectrum and Composition of the Gaseous Nebulae

3. BINARITY AND THE ABUNDANCE DISCREPANCY PROBLEM IN PLANETARY NEBULAE

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4. Low-ionization structures in planetary nebulae – II. Densities, temperatures, abundances, and excitation of six PNe;Monthly Notices of the Royal Astronomical Society;2022-09-27

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