Carbon and oxygen in H ii regions of the Magellanic Clouds: abundance discrepancy and chemical evolution-Reference-Cited by-同舟云学术

Carbon and oxygen in H ii regions of the Magellanic Clouds: abundance discrepancy and chemical evolution

Author:

Toribio San Cipriano L.¹²,Domínguez-Guzmán G.³,Esteban C.¹²,García-Rojas J.¹²,Mesa-Delgado A.⁴,Bresolin F.⁵,Rodríguez M.³,Simón-Díaz S.¹²

Affiliation:

1. Instituto de Astrofísica de Canarias, E-38200, La Laguna, Tenerife, Spain

2. Departamento de Astrofísica, Universidad de La Laguna, E-38206, La Laguna, Tenerife, Spain

3. Instituto Nacional de Astrofísica, Óptica y Electrónica, Apartado Postal 51 y 216, Puebla, Mexico

4. Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile

5. Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA

Funder

European Southern Observatory, Chile

Ministerio de Economía y Competitividad

CONACYT

FONDECYT

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference95 articles.

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