Optical spectra of radio planetary nebulae in the Small Magellanic Cloud

J. L. Payne; M. D. Filipovic; E. J. Crawford; A. Y. De Horta; G. L. White; F. H. Stootman

doi:10.2298/SAJ0876065P

Optical spectra of radio planetary nebulae in the Small Magellanic Cloud

J. L. Payne, M. D. Filipovic, E. J. Crawford, A. Y. De Horta, G. L. White, F. H. Stootman

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Abstract

We present preliminary results from spectral observations of four (4) candidate radio sources co-identified with known planetary nebulae (PNe) in the Small Magellanic Cloud (SMC). These were made using the Radcliffe 1.9-meter telescope in Sutherland, South Africa. These radio PNe were originally found in Australia Telescope Compact Array (ATCA) surveys of the SMC at 1.42 and 2.37 GHz, and were further confirmed by new high resolution ATCA images at 6 and 3 cm (4″/2″). Optical PNe and radio candidates are within 2″ and may represent a sub-population of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 M⊙ or greater, supporting the existence of PNe progenitor central stars with masses up to 8 M⊙.

Original language	English
Pages (from-to)	65-70
Number of pages	6
Journal	Serbian Astronomical Journal
Volume	176
DOIs	https://doi.org/10.2298/SAJ0876065P
Publication status	Published - 2008

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title = "Optical spectra of radio planetary nebulae in the Small Magellanic Cloud",

abstract = "We present preliminary results from spectral observations of four (4) candidate radio sources co-identified with known planetary nebulae (PNe) in the Small Magellanic Cloud (SMC). These were made using the Radcliffe 1.9-meter telescope in Sutherland, South Africa. These radio PNe were originally found in Australia Telescope Compact Array (ATCA) surveys of the SMC at 1.42 and 2.37 GHz, and were further confirmed by new high resolution ATCA images at 6 and 3 cm (4″/2″). Optical PNe and radio candidates are within 2″ and may represent a sub-population of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 M⊙ or greater, supporting the existence of PNe progenitor central stars with masses up to 8 M⊙.",

author = "Payne, {J. L.} and Filipovic, {M. D.} and Crawford, {E. J.} and {De Horta}, {A. Y.} and White, {G. L.} and Stootman, {F. H.}",

year = "2008",

doi = "10.2298/SAJ0876065P",

language = "English",

volume = "176",

pages = "65--70",

journal = "Serbian Astronomical Journal",

publisher = "Astronomical Observatory of Belgrade",

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TY - JOUR

T1 - Optical spectra of radio planetary nebulae in the Small Magellanic Cloud

AU - Payne, J. L.

AU - Filipovic, M. D.

AU - Crawford, E. J.

AU - De Horta, A. Y.

AU - White, G. L.

AU - Stootman, F. H.

PY - 2008

Y1 - 2008

N2 - We present preliminary results from spectral observations of four (4) candidate radio sources co-identified with known planetary nebulae (PNe) in the Small Magellanic Cloud (SMC). These were made using the Radcliffe 1.9-meter telescope in Sutherland, South Africa. These radio PNe were originally found in Australia Telescope Compact Array (ATCA) surveys of the SMC at 1.42 and 2.37 GHz, and were further confirmed by new high resolution ATCA images at 6 and 3 cm (4″/2″). Optical PNe and radio candidates are within 2″ and may represent a sub-population of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 M⊙ or greater, supporting the existence of PNe progenitor central stars with masses up to 8 M⊙.

AB - We present preliminary results from spectral observations of four (4) candidate radio sources co-identified with known planetary nebulae (PNe) in the Small Magellanic Cloud (SMC). These were made using the Radcliffe 1.9-meter telescope in Sutherland, South Africa. These radio PNe were originally found in Australia Telescope Compact Array (ATCA) surveys of the SMC at 1.42 and 2.37 GHz, and were further confirmed by new high resolution ATCA images at 6 and 3 cm (4″/2″). Optical PNe and radio candidates are within 2″ and may represent a sub-population of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 M⊙ or greater, supporting the existence of PNe progenitor central stars with masses up to 8 M⊙.

UR - http://handle.uws.edu.au:8081/1959.7/555936

U2 - 10.2298/SAJ0876065P

DO - 10.2298/SAJ0876065P

M3 - Article

VL - 176

SP - 65

EP - 70

JO - Serbian Astronomical Journal

JF - Serbian Astronomical Journal

ER -

Optical spectra of radio planetary nebulae in the Small Magellanic Cloud

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