Spitzer MIPS 24 μm detection of photoevaporating protoplanetary disks

Zoltan Balog; G. H. Rieke; Kate Y.L. Su; James Muzerolle; Erick T. Young

doi:10.1086/508707

Spitzer MIPS 24 μm detection of photoevaporating protoplanetary disks

Zoltan Balog
, G. H. Rieke
, Kate Y.L. Su
, James Muzerolle
, Erick T. Young

Research output: Contribution to journal › Article › peer-review

27 Scopus citations

Abstract

We present 24 μm images of three protoplanetary disks being photoevaporated around high-mass O-type stars. These objects have "cometary" structure where the dust pulled away from the disk by the photoevaporating flow is forced away from the O star by photon pressure on the dust and heating and ionization of the gas. Models of the 24 and 8 μm brightness profiles agree with this hypothesis. These models show that the mass-loss rate needed to sustain such a configuration is in agreement with or somewhat less than the theoretical predictions for the photoevaporation process.

Original language	English (US)
Pages (from-to)	L83-L86
Journal	Astrophysical Journal
Volume	650
Issue number	1 II
DOIs	https://doi.org/10.1086/508707
State	Published - Oct 10 2006

Keywords

Circumstellar matter
Planetary systems: protoplanetary disks
Stars: formation

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1086/508707

Cite this

@article{ea628579ac764bb4a380209a8c7cf7c3,

title = "Spitzer MIPS 24 μm detection of photoevaporating protoplanetary disks",

abstract = "We present 24 μm images of three protoplanetary disks being photoevaporated around high-mass O-type stars. These objects have {"}cometary{"} structure where the dust pulled away from the disk by the photoevaporating flow is forced away from the O star by photon pressure on the dust and heating and ionization of the gas. Models of the 24 and 8 μm brightness profiles agree with this hypothesis. These models show that the mass-loss rate needed to sustain such a configuration is in agreement with or somewhat less than the theoretical predictions for the photoevaporation process.",

keywords = "Circumstellar matter, Planetary systems: protoplanetary disks, Stars: formation",

author = "Zoltan Balog and Rieke, \{G. H.\} and Su, \{Kate Y.L.\} and James Muzerolle and Young, \{Erick T.\}",

note = "Funding Information: We thank the referee, John Bally, for suggestions that greatly improved the manuscript. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under NASA contract 1407. Support for this work was provided by NASA through contract 1255094, issued by JPL/ Caltech. Z. B. received support from Hungarian OTKA grants TS049872, T042509, and T049082.",

year = "2006",

month = oct,

day = "10",

doi = "10.1086/508707",

language = "English (US)",

volume = "650",

pages = "L83--L86",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1 II",

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TY - JOUR

T1 - Spitzer MIPS 24 μm detection of photoevaporating protoplanetary disks

AU - Balog, Zoltan

AU - Rieke, G. H.

AU - Su, Kate Y.L.

AU - Muzerolle, James

AU - Young, Erick T.

N1 - Funding Information: We thank the referee, John Bally, for suggestions that greatly improved the manuscript. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under NASA contract 1407. Support for this work was provided by NASA through contract 1255094, issued by JPL/ Caltech. Z. B. received support from Hungarian OTKA grants TS049872, T042509, and T049082.

PY - 2006/10/10

Y1 - 2006/10/10

N2 - We present 24 μm images of three protoplanetary disks being photoevaporated around high-mass O-type stars. These objects have "cometary" structure where the dust pulled away from the disk by the photoevaporating flow is forced away from the O star by photon pressure on the dust and heating and ionization of the gas. Models of the 24 and 8 μm brightness profiles agree with this hypothesis. These models show that the mass-loss rate needed to sustain such a configuration is in agreement with or somewhat less than the theoretical predictions for the photoevaporation process.

AB - We present 24 μm images of three protoplanetary disks being photoevaporated around high-mass O-type stars. These objects have "cometary" structure where the dust pulled away from the disk by the photoevaporating flow is forced away from the O star by photon pressure on the dust and heating and ionization of the gas. Models of the 24 and 8 μm brightness profiles agree with this hypothesis. These models show that the mass-loss rate needed to sustain such a configuration is in agreement with or somewhat less than the theoretical predictions for the photoevaporation process.

KW - Circumstellar matter

KW - Planetary systems: protoplanetary disks

KW - Stars: formation

UR - https://www.scopus.com/pages/publications/33751435970

UR - https://www.scopus.com/pages/publications/33751435970#tab=citedBy

U2 - 10.1086/508707

DO - 10.1086/508707

M3 - Article

AN - SCOPUS:33751435970

SN - 0004-637X

VL - 650

SP - L83-L86

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 II

ER -

Spitzer MIPS 24 μm detection of photoevaporating protoplanetary disks

Abstract

Keywords

ASJC Scopus subject areas

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