Published July 1988
| Version v1
Journal article
Linear polarization observations in selected celestial zones - the central region of our Galaxy
- 1. National Research Council of Canada, Herzberg Institute of Astrophysics, Ottawa
- 2. Northern Telecom Electronics, Ltd., Ottawa (Canada)
- 3. National Radio Astronomy Observatory, Socorro, NM (USA)
Description
The Algonquin Radio Observatory and the very large array have been used to obtain the linear polarization integrated over the angular size of a radio galaxy or quasar. All sources are located in a celestial angular zone encompassing the central region of the Galaxy. In addition to the total intensity (Stokes I) flux density, the percentage and position angle of the linear polarization (Stokes Q and U) are obtained for 14 sources at several centimetric wavelengths. 15 references
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal, Supplement Series
- Journal Volume
- 67
- Series
- Astrophys. J., Suppl. Ser.
- Journal Page Range
- 279-282
- ISSN
- 0067-0049
- CODEN
- APJSA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20001026
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC RADIO SOURCES; GALAXY NUCLEI; INTERSTELLAR MAGNETIC FIELDS; MILKY WAY; POLARIZATION; QUASARS; RADIO GALAXIES; RADIOWAVE RADIATION
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; GALAXIES; MAGNETIC FIELDS; RADIATIONS