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Condition for low-mass star formation in shock-compressed metal-poor clouds

  • Published:2018-07-19 Issue:1 Volume:480 Page:1043-1056
  • ISSN:0035-8711
  • Container-title:Monthly Notices of the Royal Astronomical Society
  • language:en
  • Short-container-title:

Author:

Nakauchi Daisuke1,Omukai Kazuyuki1,Schneider Raffaella23

Affiliation:

1. Astronomical Institute, Tohoku University, Aoba, Sendai 980-8578, Japan

2. Dipartimento di Fisica, Universitá di Roma ‘La Sapienza’, P.le Aldo Moro 2, I-00185 Roma, Italy

3. INAF/Osservatorio Astronomico di Roma, Via Frascati 33, Monte Porzio Catone, I-00078 Roma, Italy

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 4 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. Ionization degree and magnetic diffusivity in star-forming clouds with different metallicities;Monthly Notices of the Royal Astronomical Society;2021-01-29

2. From hydrodynamics to N-body simulations of star clusters: mergers and rotation;Monthly Notices of the Royal Astronomical Society;2020-12-05

3. Making a Supermassive Star by Stellar Bombardment;The Astrophysical Journal;2020-03-20

4. Erratum: Condition for low-mass star formation in shock-compressed metal-poor clouds;Monthly Notices of the Royal Astronomical Society;2018-12-08
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