Probing X-ray photoevaporative winds through their interaction with ionizing radiation in cluster environments: the case for X-ray proplyds
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/446/3/2944/10447688/stu2248.pdf
Reference43 articles.
1. Disks, Microjets, Windblown Bubbles, and Outflows in the Orion Nebula
2. Spitzer MIPS 24 μm Detection of Photoevaporating Protoplanetary Disks
3. [ITAL]HST[/ITAL]/WFPC2 and VLT/ISAAC Observations of Proplyds in the Giant H [CSC]ii[/CSC] Region NGC 3603
4. 2.12 Micron Molecular Hydrogen Emission from Circumstellar Disks Embedded in the Orion Nebula
5. Solar system-sized condensations in the Orion Nebula
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1. The VLT MUSE NFM view of outflows and externally photoevaporating discs near the orion bar★;Monthly Notices of the Royal Astronomical Society;2023-08-25
2. A solution to the proplyd lifetime problem;Monthly Notices of the Royal Astronomical Society;2019-09-16
3. How Do Disks and Planetary Systems in High-mass Open Clusters Differ from Those around Field Stars?;The Astrophysical Journal;2018-11-13
4. PROPLYDS AROUND A B1 STAR: 42 ORIONIS IN NGC 1977;The Astrophysical Journal;2016-07-20
5. M STARS IN THE TW HYA ASSOCIATION: STELLAR X-RAYS AND DISK DISSIPATION;The Astronomical Journal;2016-06-13
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