The UM/CTIO magellanic cloud emission-line survey

R. Chris Smith; J. Bregman; Y. H. Chu; R. Ciardullo; G. Jacoby; R. Kennicutt; S. Oey; F. Winkler; D. Zaritsky

doi:10.1071/AS98163

The UM/CTIO magellanic cloud emission-line survey

R. Chris Smith, J. Bregman, Y. H. Chu, R. Ciardullo, G. Jacoby, R. Kennicutt, S. Oey, F. Winkler, D. Zaritsky

Research output: Contribution to journal › Review article › peer-review

49 Scopus citations

Abstract

The Magellanic Clouds are unique in providing us with sites to study the interstellar medium (ISM) and its components at all scales. To promote the pursuit of such studies, we have begun the Magellanic Cloud Emission-line Survey (MCELS), a deep imaging survey of both of these nearby galaxies in the emission of Hα, [SII], and [OIII]. The emission-line images will be used in detailed optical and multiwavelength studies of HII regions, supernova remnants, planetary nebulae, superbubbles, and supergiant shells. Together with parallel surveys at other wavelengths, this survey will provide the foundation upon which to build a deeper understanding of the ISM in the Clouds and other galaxies, from small scales (∼1 pc) all the way up to global scales.

Original language	English (US)
Pages (from-to)	163-164
Number of pages	2
Journal	Publications of the Astronomical Society of Australia
Volume	15
Issue number	1
DOIs	https://doi.org/10.1071/AS98163
State	Published - Apr 1998

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1071/AS98163

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title = "The UM/CTIO magellanic cloud emission-line survey",

abstract = "The Magellanic Clouds are unique in providing us with sites to study the interstellar medium (ISM) and its components at all scales. To promote the pursuit of such studies, we have begun the Magellanic Cloud Emission-line Survey (MCELS), a deep imaging survey of both of these nearby galaxies in the emission of Hα, [SII], and [OIII]. The emission-line images will be used in detailed optical and multiwavelength studies of HII regions, supernova remnants, planetary nebulae, superbubbles, and supergiant shells. Together with parallel surveys at other wavelengths, this survey will provide the foundation upon which to build a deeper understanding of the ISM in the Clouds and other galaxies, from small scales (∼1 pc) all the way up to global scales.",

author = "Smith, {R. Chris} and J. Bregman and Chu, {Y. H.} and R. Ciardullo and G. Jacoby and R. Kennicutt and S. Oey and F. Winkler and D. Zaritsky",

year = "1998",

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doi = "10.1071/AS98163",

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T1 - The UM/CTIO magellanic cloud emission-line survey

AU - Smith, R. Chris

AU - Bregman, J.

AU - Chu, Y. H.

AU - Ciardullo, R.

AU - Jacoby, G.

AU - Kennicutt, R.

AU - Oey, S.

AU - Winkler, F.

AU - Zaritsky, D.

PY - 1998/4

Y1 - 1998/4

N2 - The Magellanic Clouds are unique in providing us with sites to study the interstellar medium (ISM) and its components at all scales. To promote the pursuit of such studies, we have begun the Magellanic Cloud Emission-line Survey (MCELS), a deep imaging survey of both of these nearby galaxies in the emission of Hα, [SII], and [OIII]. The emission-line images will be used in detailed optical and multiwavelength studies of HII regions, supernova remnants, planetary nebulae, superbubbles, and supergiant shells. Together with parallel surveys at other wavelengths, this survey will provide the foundation upon which to build a deeper understanding of the ISM in the Clouds and other galaxies, from small scales (∼1 pc) all the way up to global scales.

AB - The Magellanic Clouds are unique in providing us with sites to study the interstellar medium (ISM) and its components at all scales. To promote the pursuit of such studies, we have begun the Magellanic Cloud Emission-line Survey (MCELS), a deep imaging survey of both of these nearby galaxies in the emission of Hα, [SII], and [OIII]. The emission-line images will be used in detailed optical and multiwavelength studies of HII regions, supernova remnants, planetary nebulae, superbubbles, and supergiant shells. Together with parallel surveys at other wavelengths, this survey will provide the foundation upon which to build a deeper understanding of the ISM in the Clouds and other galaxies, from small scales (∼1 pc) all the way up to global scales.

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The UM/CTIO magellanic cloud emission-line survey

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