Disc wind models for FU Ori objects-Reference-Cited by-同舟云学术

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Disc wind models for FU Ori objects

Published:2018-11-28 Issue:2 Volume:483 Page:1663-1673
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Milliner Kelly¹,Matthews James H²^ORCID,Long Knox S³,Hartmann Lee¹^ORCID

Affiliation:

1. Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48105, USA

2. University of Oxford, Astrophysics, Keble Road, Oxford OX1 3RH, UK

3. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA

Funder

University of Michigan

National Science Foundation

Science and Technology Facilities Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/483/2/1663/27099008/sty3197.pdf

Reference66 articles.

1. The effects of X-ray photoionization and heating on the structure of circumstellar discs

2. Locating the Launching Region of T Tauri Winds: The Case of DG Tauri

3. TOWARD A GLOBAL EVOLUTIONARY MODEL OF PROTOPLANETARY DISKS

4. WIND-DRIVEN ACCRETION IN PROTOPLANETARY DISKS. I. SUPPRESSION OF THE MAGNETOROTATIONAL INSTABILITY AND LAUNCHING OF THE MAGNETOCENTRIFUGAL WIND

5. Instability, turbulence, and enhanced transport in accretion disks

Cited by 14 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. An Expanding Accretion Disk and a Warm Disk Wind as Seen in the Spectral Evolution of HBC 722;The Astrophysical Journal;2024-08-01

2. Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FU Orionis;The Astrophysical Journal;2024-04-29

3. Disk Cooling and Wind Lines as Seen in the Spectral Line Evolution of V960 Mon;The Astrophysical Journal;2023-11-20

4. Gaia21bty: An EXor light curve exhibiting a FUor spectrum;Monthly Notices of the Royal Astronomical Society;2023-07-18

5. Diagnosing FU Ori-like Sources: The Parameter Space of Viscously Heated Disks in the Optical and Near-infrared;The Astrophysical Journal;2022-09-01

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