Using the 1.4 GHz NRAO VLA Sky Survey (NVSS) images and source catalog, we identified 315 radio sources stronger than approximate to 2.5 mJy among over 1000 recently discovered planetary nebulae north of J2000 declination delta = - 40 degrees. Two-thirds of these radio sources are weaker than 10 mJy at 1.4 GHz. This result is a uniform supplement to the previous NVSS radio identification of known PNe and a large homogeneous sample including over 1000 PNe with NVSS sources is obtained. By examining the radio properties of PNe, it is found that most of the planetary nebulae detected at both 1.4 and 5.0 GHz are optically thick at lambda = 20 cm.Astronomy & AstrophysicsSCI(E)7ARTICLE2282-28715
We report on radio continuum observations of unidentified IRAS point sources with far IR colors that...
We present preliminary results from spectral observations of four (4) candidate radio sources co-ide...
We present 11 spectra from 12 candidate radio sources co-identified with known planetary nebulae (PN...
We present an updated and newly compiled radio-continuum data base for Macquarie/AAO/Strasbourg Hα (...
© 2015 The Authors. We provide radio spectral properties at high frequencies (1=v (GHz) = 20) for 65...
We have used the Cornish radio catalogue combined with the use of multiwavelength data to identify 6...
We report an Australia Telescope Compact Array (ATCA) radio-continuum observations of 26 planetary n...
This research presents a new radio-selected sample of compact Galactic PNe from the CORNISH survey, ...
International audienceAims: The aim of this study is to investigate the physical properties of molec...
We report an Australia Telescope Compact Array (ATCA) radio-continuum observations of 26 planetary n...
Aims. The aim of this study is to investigate the physical properties of molecular envelopes of plan...
We have used the Cornish radio catalogue combined with the use of multiwavelength data to identify 6...
We have analysed the radio fluxes for 264 planetary nebulae for which reliable measurements of fluxe...
We present 11 spectra from 12 candidate radio sources co-identified with known planetary nebulae (PN...
We report the extragalactic radio-continuum detection of 15 planetary nebulae (PNe) in the Magellani...
We report on radio continuum observations of unidentified IRAS point sources with far IR colors that...
We present preliminary results from spectral observations of four (4) candidate radio sources co-ide...
We present 11 spectra from 12 candidate radio sources co-identified with known planetary nebulae (PN...
We present an updated and newly compiled radio-continuum data base for Macquarie/AAO/Strasbourg Hα (...
© 2015 The Authors. We provide radio spectral properties at high frequencies (1=v (GHz) = 20) for 65...
We have used the Cornish radio catalogue combined with the use of multiwavelength data to identify 6...
We report an Australia Telescope Compact Array (ATCA) radio-continuum observations of 26 planetary n...
This research presents a new radio-selected sample of compact Galactic PNe from the CORNISH survey, ...
International audienceAims: The aim of this study is to investigate the physical properties of molec...
We report an Australia Telescope Compact Array (ATCA) radio-continuum observations of 26 planetary n...
Aims. The aim of this study is to investigate the physical properties of molecular envelopes of plan...
We have used the Cornish radio catalogue combined with the use of multiwavelength data to identify 6...
We have analysed the radio fluxes for 264 planetary nebulae for which reliable measurements of fluxe...
We present 11 spectra from 12 candidate radio sources co-identified with known planetary nebulae (PN...
We report the extragalactic radio-continuum detection of 15 planetary nebulae (PNe) in the Magellani...
We report on radio continuum observations of unidentified IRAS point sources with far IR colors that...
We present preliminary results from spectral observations of four (4) candidate radio sources co-ide...
We present 11 spectra from 12 candidate radio sources co-identified with known planetary nebulae (PN...