Study of the extended radio emission of two supernova remnants and four planetary nebulae associated with MIPSGAL bubbles

A. Ingallinera, C. Trigilio, G. Umana, P. Leto, C. Agliozzo, C. Buemi

Research output: Contribution to journalArticle

9 Citations (Scopus)

Abstract

We present radio observations, made using theVery Large Array and the Green BankTelescope, of two supernova remnants and four planetary nebulae. These objects are part of a larger sample of radio sources, discussed in a previous paper, a counterpart of the MIPSGAL 24-μmcompact bubbles. For the two supernova remnants, we have combined the interferometric observations with single-dish data to obtain both a high resolution and a good sensitivity to extended structures. We discuss in detail the entire combination procedure adopted and the reliability of the resulting maps. For one supernova remnant, we pose a more stringent upper limit for the flux density of its undetected pulsar, and we also show prominent spectral index spatial variations, probably resulting either from inhomogeneities in the magnetic field and in its ejecta or from an interaction between the supernova shock and molecular clouds. We eventually use the 5-GHz maps of the four planetary nebulae to estimate their distances and their ionized masses.

Original languageEnglish
Pages (from-to)4504-4514
Number of pages11
JournalMonthly Notices of the Royal Astronomical Society
Volume445
Issue number4
DOIs
Publication statusPublished - 29 Sep 2014

Fingerprint

planetary nebulae
supernova remnants
radio emission
bubble
bubbles
radio
ejecta
inhomogeneity
spatial variation
radio observation
parabolic reflectors
magnetic field
molecular clouds
pulsars
supernovae
flux density
shock
sensitivity
high resolution
estimates

Keywords

  • ISM: supernova remnants
  • Planetary nebulae: general
  • Techniques: image processing

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Ingallinera, A. ; Trigilio, C. ; Umana, G. ; Leto, P. ; Agliozzo, C. ; Buemi, C. / Study of the extended radio emission of two supernova remnants and four planetary nebulae associated with MIPSGAL bubbles. In: Monthly Notices of the Royal Astronomical Society. 2014 ; Vol. 445, No. 4. pp. 4504-4514.
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Study of the extended radio emission of two supernova remnants and four planetary nebulae associated with MIPSGAL bubbles. / Ingallinera, A.; Trigilio, C.; Umana, G.; Leto, P.; Agliozzo, C.; Buemi, C.

In: Monthly Notices of the Royal Astronomical Society, Vol. 445, No. 4, 29.09.2014, p. 4504-4514.

Research output: Contribution to journalArticle

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AU - Ingallinera, A.

AU - Trigilio, C.

AU - Umana, G.

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AU - Agliozzo, C.

AU - Buemi, C.

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AB - We present radio observations, made using theVery Large Array and the Green BankTelescope, of two supernova remnants and four planetary nebulae. These objects are part of a larger sample of radio sources, discussed in a previous paper, a counterpart of the MIPSGAL 24-μmcompact bubbles. For the two supernova remnants, we have combined the interferometric observations with single-dish data to obtain both a high resolution and a good sensitivity to extended structures. We discuss in detail the entire combination procedure adopted and the reliability of the resulting maps. For one supernova remnant, we pose a more stringent upper limit for the flux density of its undetected pulsar, and we also show prominent spectral index spatial variations, probably resulting either from inhomogeneities in the magnetic field and in its ejecta or from an interaction between the supernova shock and molecular clouds. We eventually use the 5-GHz maps of the four planetary nebulae to estimate their distances and their ionized masses.

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