Observing substructure in circumstellar discs around massive young stellar objects-Reference-Cited by-同舟云学术

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Observing substructure in circumstellar discs around massive young stellar objects

Published:2018-11-10 Issue:4 Volume:482 Page:4673-4686
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Jankovic M R¹,Haworth T J¹^ORCID,Ilee J D²³^ORCID,Forgan D H⁴^ORCID,Cyganowski C J⁴^ORCID,Walsh C³,Brogan C L⁵,Hunter T R⁵,Mohanty S¹

Affiliation:

1. Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, UK

2. Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK

3. School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK

4. SUPA, School of Physics, Astronomy, University of St Andrews, North Haugh, St Andrews, Scotland KY16 9SS, UK

5. NRAO, 520 Edgemont Rd, Charlottesville, VA 22903, USA

Funder

JDI

European Research Council

Science and Technology Facilities Council

National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/482/4/4673/26779163/sty3038.pdf

Reference87 articles.

1. Using FU Orionis outbursts to constrain self-regulated protostellar disk models

2. Rotating toroids in G10.62–0.38, G19.61–0.23, and G29.96–0.02

3. Kinematics of a Hot Massive Accretion Disk Candidate

4. Fragmentation and disk formation in high-mass star formation: The ALMA view of G351.77-0.54 at 0.06′′ resolution

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2. A small survey for massive stars in the LMC/SMC: binaries and pulsations;Monthly Notices of the Royal Astronomical Society;2023-05-22

3. A Keplerian disk with a four-arm spiral birthing an episodically accreting high-mass protostar;Nature Astronomy;2023-02-27

4. The burst mode of accretion in massive star formation with stellar inertia;Monthly Notices of the Royal Astronomical Society;2022-10-16

5. A Multitransition Methanol Maser Study of the Accretion Burst Source G358.93–0.03-MM1;The Astronomical Journal;2022-01-24

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