Submillimetre photometry of post-asymptotic giant branch stars

T. Gledhill; I. Bains; J.A. Yates

doi:10.1046/j.1365-8711.2002.05550.x

Submillimetre photometry of post-asymptotic giant branch stars

T. Gledhill
, I. Bains
, J.A. Yates

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

15 Citations (Scopus)

Abstract

Stars in the post-asymptotic giant branch (post-AGB) phase of evolution are surrounded by detached circumstellar envelopes containing dust which emits thermally in the mid- and far-infrared. Here we present 850-μm SCUBA photometry of nine candidate post-AGB stars. All targets are detected at 850 μm and we use these fluxes to estimate the envelope dust masses and, by comparison with the 100-μm IRAS fluxes, the dust emissivity index.

Original language	English
Pages (from-to)	L55-L58
Journal	Monthly Notices of the Royal Astronomical Society (MNRAS)
Volume	332
Issue number	3
DOIs	https://doi.org/10.1046/j.1365-8711.2002.05550.x
Publication status	Published - 2002

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10.1046/j.1365-8711.2002.05550.x

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title = "Submillimetre photometry of post-asymptotic giant branch stars",

abstract = "Stars in the post-asymptotic giant branch (post-AGB) phase of evolution are surrounded by detached circumstellar envelopes containing dust which emits thermally in the mid- and far-infrared. Here we present 850-μm SCUBA photometry of nine candidate post-AGB stars. All targets are detected at 850 μm and we use these fluxes to estimate the envelope dust masses and, by comparison with the 100-μm IRAS fluxes, the dust emissivity index.",

author = "T. Gledhill and I. Bains and J.A. Yates",

note = "{\textquoteleft}The definitive version is available at www.blackwell-synergy.com '. Copyright Royal Astronomical Society. DOI: 10.1046/j.1365-8711.2002.05550.x [Full text of this article is not available in the UHRA]",

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doi = "10.1046/j.1365-8711.2002.05550.x",

language = "English",

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T1 - Submillimetre photometry of post-asymptotic giant branch stars

AU - Gledhill, T.

AU - Bains, I.

AU - Yates, J.A.

N1 - ‘The definitive version is available at www.blackwell-synergy.com '. Copyright Royal Astronomical Society. DOI: 10.1046/j.1365-8711.2002.05550.x [Full text of this article is not available in the UHRA]

PY - 2002

Y1 - 2002

N2 - Stars in the post-asymptotic giant branch (post-AGB) phase of evolution are surrounded by detached circumstellar envelopes containing dust which emits thermally in the mid- and far-infrared. Here we present 850-μm SCUBA photometry of nine candidate post-AGB stars. All targets are detected at 850 μm and we use these fluxes to estimate the envelope dust masses and, by comparison with the 100-μm IRAS fluxes, the dust emissivity index.

AB - Stars in the post-asymptotic giant branch (post-AGB) phase of evolution are surrounded by detached circumstellar envelopes containing dust which emits thermally in the mid- and far-infrared. Here we present 850-μm SCUBA photometry of nine candidate post-AGB stars. All targets are detected at 850 μm and we use these fluxes to estimate the envelope dust masses and, by comparison with the 100-μm IRAS fluxes, the dust emissivity index.

U2 - 10.1046/j.1365-8711.2002.05550.x

DO - 10.1046/j.1365-8711.2002.05550.x

M3 - Article

SN - 0035-8711

VL - 332

SP - L55-L58

JO - Monthly Notices of the Royal Astronomical Society (MNRAS)

JF - Monthly Notices of the Royal Astronomical Society (MNRAS)

IS - 3

ER -

Submillimetre photometry of post-asymptotic giant branch stars

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