Physical properties of superbubbles in the Antennae galaxies

Author:

Camps-Fariña A.12,Zaragoza-Cardiel J.3,Beckman J. E.124,Font J.12,Velázquez P. F.5,Rodríguez-González A.5,Rosado M.3

Affiliation:

1. Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, E-38205 La Laguna, Tenerife, Spain

2. Department of Astrophysics, University of La Laguna, E-38205 La Laguna, Tenerife, Spain

3. Instituto de Astronomía, Universidad Nacional Autónoma de México, Apartado Postal 70-264, CP 04510 México D.F., México

4. CSIC, C/ Serrano, 117, 28006, Madrid, Spain

5. Instituto de Ciencias Nucleares, Universidad Nacional de México, Apartado Postal 70-264, CP 04510 México D.F., México

Funder

MINECO

REA

UNAM

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 5 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Quantifying the energetics of molecular superbubbles in PHANGS galaxies;Astronomy & Astrophysics;2023-08

2. Hα kinematics of superbubbles and supernova remnants of the dwarf galaxy NGC 4214;Monthly Notices of the Royal Astronomical Society;2023-07-07

3. Stars made in outflows may populate the stellar halo of the Milky Way;Monthly Notices of the Royal Astronomical Society;2020-03-03

4. The fraction of ionizing radiation from massive stars that escapes to the intergalactic medium;Monthly Notices of the Royal Astronomical Society;2018-12-20

5. Origin of Hot Bubble in NGC 6822 Hubble V Star-Forming Region;Proceedings of the International Astronomical Union;2018-08

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