The dark lane of the bipolar nebula NGC 6302

M. Matsuura; A. A. Zijlstra; G. A. Fuller

doi:10.1063/1.2146277

The dark lane of the bipolar nebula NGC 6302

M. Matsuura, A. A. Zijlstra, G. A. Fuller

Research output: Chapter in Book/Conference proceeding › Conference contribution

Abstract

The butterfly-shaped planetary nebula, NGC 6302, shows a dense equatorial dark lane, which is presumably a dusty disc. We report observations of the dark lane based on Hubble Space Telescope (HST) Hα image, James Clerk Maxwell Telescope (JCMT) 450 μm images, and JCMT 12CO, 13CO J=2-1 and 3-2 line observations. © 2005 American Institute of Physics.

Original language	English
Title of host publication	AIP Conference Proceedings\|AIP Conf. Proc.
Pages	211
Volume	804
DOIs	https://doi.org/10.1063/1.2146277
Publication status	Published - 28 Nov 2005
Event	International Conference on Planetary Nebulae as Astronomical Tools - Gdansk Duration: 28 Nov 2005 → …

Conference

Conference	International Conference on Planetary Nebulae as Astronomical Tools
City	Gdansk
Period	28/11/05 → …

Keywords

(ISM:)dust, extinction
(ISM:)Planetary nebulae:individual:NGC 6302
ISM: jets and outflows

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10.1063/1.2146277

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title = "The dark lane of the bipolar nebula NGC 6302",

abstract = "The butterfly-shaped planetary nebula, NGC 6302, shows a dense equatorial dark lane, which is presumably a dusty disc. We report observations of the dark lane based on Hubble Space Telescope (HST) Hα image, James Clerk Maxwell Telescope (JCMT) 450 μm images, and JCMT 12CO, 13CO J=2-1 and 3-2 line observations. {\textcopyright} 2005 American Institute of Physics.",

keywords = "(ISM:)dust, extinction, (ISM:)Planetary nebulae:individual:NGC 6302, ISM: jets and outflows",

author = "M. Matsuura and Zijlstra, {A. A.} and Fuller, {G. A.}",

year = "2005",

month = nov,

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doi = "10.1063/1.2146277",

language = "English",

isbn = "0735402949",

volume = "804",

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AU - Zijlstra, A. A.

AU - Fuller, G. A.

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N2 - The butterfly-shaped planetary nebula, NGC 6302, shows a dense equatorial dark lane, which is presumably a dusty disc. We report observations of the dark lane based on Hubble Space Telescope (HST) Hα image, James Clerk Maxwell Telescope (JCMT) 450 μm images, and JCMT 12CO, 13CO J=2-1 and 3-2 line observations. © 2005 American Institute of Physics.

AB - The butterfly-shaped planetary nebula, NGC 6302, shows a dense equatorial dark lane, which is presumably a dusty disc. We report observations of the dark lane based on Hubble Space Telescope (HST) Hα image, James Clerk Maxwell Telescope (JCMT) 450 μm images, and JCMT 12CO, 13CO J=2-1 and 3-2 line observations. © 2005 American Institute of Physics.

KW - (ISM:)dust, extinction

KW - (ISM:)Planetary nebulae:individual:NGC 6302

KW - ISM: jets and outflows

U2 - 10.1063/1.2146277

DO - 10.1063/1.2146277

M3 - Conference contribution

SN - 0735402949

SN - 9780735402942

VL - 804

SP - 211

BT - AIP Conference Proceedings|AIP Conf. Proc.

T2 - International Conference on Planetary Nebulae as Astronomical Tools

Y2 - 28 November 2005

ER -

The dark lane of the bipolar nebula NGC 6302

Abstract

Conference

Keywords

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