SIMBAD references

2011MNRAS.412..223B - Mon. Not. R. Astron. Soc., 412, 223-245 (2011/March-3)

Radio-continuum detections of galactic planetary nebulae – I. MASH PNe detected in large-scale radio surveys.


Abstract (from CDS):

We present an updated and newly compiled radio-continuum data base for Macquarie/AAO/Strasbourg Hα (MASH) planetary nebulae (PNe) detected in the extant large-scale `blind' radio-continuum surveys [NRAO VLA Sky Survey (NVSS), Sydney University Molonglo Sky Survey/Molonglo Galactic Plane Surveys (SUMSS/MGPS-2) and Parkes-MIT-NRAO (PMN)] and, for a small number of MASH PNe, observed and detected in targeted radio-continuum observations. We found radio counterparts for approximately 250 MASH PNe. In comparison with the percentage of previously known Galactic PNe detected in the NVSS and MGPS-2 radio-continuum surveys and according to their position on the flux density angular diameter and the radio brightness temperature evolutionary diagrams we conclude, unsurprisingly, that the MASH sample presents the radio-faint end of the known Galactic PNe population. Also, we present radio-continuum spectral properties of a small sub-sample of MASH PNe located in the strip between declinations -30° and -40°, that are detected in both the NVSS and MGPS-2 radio surveys.

Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS

Journal keyword(s): radiation mechanisms: thermal - astronomical data bases: miscellaneous - planetary nebulae: general - radio continuum: ISM

VizieR on-line data: <Available at CDS (J/MNRAS/412/223): table1.dat table2.dat table3.dat table4.dat notes.dat>

Simbad objects: 289

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2011MNRAS.412..223B and select 'bookmark this link' or equivalent in the popup menu


© Université de Strasbourg/CNRS

    • Contact