Radio-continuum sources in nearby and bright E/S0 galaxies - Sample selection and well-studied cases
Abstract
A volume-limited sample of 216 nearby and optically bright E/S0 galaxies has been compiled. Twelve of the galaxies are confirmed radio sources for which VLA images are available. Most of the remaining galaxies have powers less than or of the order of 10 to the 21st-22nd W/Hz, and this information is used to establish the parameters of a new VLA survey of these galaxies. The basic optical properties of the galaxies in the sample are tabulated. 102 refs.
- Authors:
-
- New Mexico Institute of Mining and Technology, Socorro (USA)
- Publication Date:
- OSTI Identifier:
- 5993631
- Resource Type:
- Journal Article
- Journal Name:
- Astronomical Journal; (USA)
- Additional Journal Information:
- Journal Volume: 101; Journal ID: ISSN 0004-6256
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; GALAXIES; RADIOWAVE RADIATION; COSMIC RADIO SOURCES; ELLIPTICAL CONFIGURATION; OPTICAL PROPERTIES; CONFIGURATION; ELECTROMAGNETIC RADIATION; PHYSICAL PROPERTIES; RADIATIONS; 640105* - Astrophysics & Cosmology- Galaxies
Citation Formats
Wrobel, J M. Radio-continuum sources in nearby and bright E/S0 galaxies - Sample selection and well-studied cases. United States: N. p., 1991.
Web. doi:10.1086/115673.
Wrobel, J M. Radio-continuum sources in nearby and bright E/S0 galaxies - Sample selection and well-studied cases. United States. https://doi.org/10.1086/115673
Wrobel, J M. 1991.
"Radio-continuum sources in nearby and bright E/S0 galaxies - Sample selection and well-studied cases". United States. https://doi.org/10.1086/115673.
@article{osti_5993631,
title = {Radio-continuum sources in nearby and bright E/S0 galaxies - Sample selection and well-studied cases},
author = {Wrobel, J M},
abstractNote = {A volume-limited sample of 216 nearby and optically bright E/S0 galaxies has been compiled. Twelve of the galaxies are confirmed radio sources for which VLA images are available. Most of the remaining galaxies have powers less than or of the order of 10 to the 21st-22nd W/Hz, and this information is used to establish the parameters of a new VLA survey of these galaxies. The basic optical properties of the galaxies in the sample are tabulated. 102 refs.},
doi = {10.1086/115673},
url = {https://www.osti.gov/biblio/5993631},
journal = {Astronomical Journal; (USA)},
issn = {0004-6256},
number = ,
volume = 101,
place = {United States},
year = {Tue Jan 01 00:00:00 EST 1991},
month = {Tue Jan 01 00:00:00 EST 1991}
}
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