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The Coordinated Radio and Infrared Survey for High-mass Star Formation. IV: A new radio selected sample of compact Galactic Planetary Nebulae
by
Oudmaijer, R D
, Purcell, C R
, Irabor, T
, Hoare, M G
, Zijlstra, A A
, Kurtz, S
, Umana, G
, Lumsden, S L
, Urquhart, J S
in
Aerial surveys
/ Biological evolution
/ Diagnostic systems
/ Extinction
/ Massive stars
/ Nebulae
/ Planet formation
/ Planetary nebulae
/ Radio emission
/ Star & galaxy formation
/ Star formation
2018
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The Coordinated Radio and Infrared Survey for High-mass Star Formation. IV: A new radio selected sample of compact Galactic Planetary Nebulae
by
Oudmaijer, R D
, Purcell, C R
, Irabor, T
, Hoare, M G
, Zijlstra, A A
, Kurtz, S
, Umana, G
, Lumsden, S L
, Urquhart, J S
in
Aerial surveys
/ Biological evolution
/ Diagnostic systems
/ Extinction
/ Massive stars
/ Nebulae
/ Planet formation
/ Planetary nebulae
/ Radio emission
/ Star & galaxy formation
/ Star formation
2018
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Do you wish to request the book?
The Coordinated Radio and Infrared Survey for High-mass Star Formation. IV: A new radio selected sample of compact Galactic Planetary Nebulae
by
Oudmaijer, R D
, Purcell, C R
, Irabor, T
, Hoare, M G
, Zijlstra, A A
, Kurtz, S
, Umana, G
, Lumsden, S L
, Urquhart, J S
in
Aerial surveys
/ Biological evolution
/ Diagnostic systems
/ Extinction
/ Massive stars
/ Nebulae
/ Planet formation
/ Planetary nebulae
/ Radio emission
/ Star & galaxy formation
/ Star formation
2018
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The Coordinated Radio and Infrared Survey for High-mass Star Formation. IV: A new radio selected sample of compact Galactic Planetary Nebulae
Paper
The Coordinated Radio and Infrared Survey for High-mass Star Formation. IV: A new radio selected sample of compact Galactic Planetary Nebulae
2018
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Overview
We present a new radio-selected sample of PNe from the CORNISH survey. This is a radio continuum survey of the inner Galactic plane covering Galactic longitude, \\(10^\\circ 1000 K) and located closer than 7 kpc. Within this sample is a water-maser PN with a spectral index of \\(-0.55\\pm 0.08\\), which indicates non-thermal radio emission. Such a radio-selected sample, unaffected by extinction, will be particularly useful to compare with population synthesis models and should contribute to the understanding of the formation and evolution of PNe.
Publisher
Cornell University Library, arXiv.org
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