A model for a photoionized, conical jet from a young, massive star-Reference-Cited by-同舟云学术

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A model for a photoionized, conical jet from a young, massive star

Published:2017-08-02 Issue:4 Volume:471 Page:4910-4916
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Raga A. C.¹,Cantó J.²,Tinoco-Arenas A.³,Rodríguez-Ramírez J. C.¹,Rodríguez L. F.⁴,Lizano S.⁴

Affiliation:

1. Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Ap. 70-543, 04510 Cd. Mx., Mexico

2. Instituto de Astronomía, Universidad Nacional Autónoma de México, Ap. 70-468, 04510 Cd. Mx., Mexico

3. Instituto de Geofísica, Universidad Nacional Autónoma de México, 04510 Cd. Mx., Mexico

4. Instituto de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, A.P. 3-72 (Xangari), 58089 Morelia, Michoacán, Mexico

Funder

CONACyT

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/471/4/4910/19650191/stx1938.pdf

Reference33 articles.

1. A search for shock-excited optical emission from the outflows of massive young stellar objects

2. The Irradiated Herbig‐Haro Jets Near σ Orionis

3. Irradiated Jets and Outflows in the Pelican Nebula

4. Accretion disks in luminous young stellar objects

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