| 1. |
- Bååth, L.B. 1948-, et al.
(author)
-
High Resolution Observations of the QSO 3C 345 at 1.3 centimeters
- 1981
-
In: Astrophysical Journal. - Philadelphia, PA : Institute of Physics Publishing (IOPP). - 0004-637X .- 1538-4357. ; 243, s. L123-L126
-
Journal article (peer-reviewed)abstract
- High-resolution VLBI observations made at a frequency of 22.235 GHz of the quasar 3C 345 are discussed. Antennas located at the Crimean Astrophysical Observatory, USSR; Onsala, Sweden; Effelsberg, West Germany; and the Haystack Observatory, Massachusetts were employed at 4-min integration times to provide baselines ranging up to 5.5 x 10 to the 8th wavelengths. About 40% of the total flux density of 7.85 Jy, observed in November 1977, and 8.05 Jy, observed in October 1978, is found to originate in an unresolved component of the quasar core in a region less than 0.1 milliarcsec in diameter. The elongated jet-like component of the quasar is observed to contain several peaks of emission extending up to 6 milliarsec from the core which decreased in extent between the two observations.
|
|
| 2. |
- Giuffrida, T.S., et al.
(author)
-
VLBI Studies of the W3OH Water Maser
- 1977
-
In: Bulletin of the American Astronomical Society. - New York, NY : American Institute of Physics (AIP). - 0002-7537 .- 2330-9458. ; 9, s. 576-576
-
Journal article (peer-reviewed)
|
|
| 3. |
- Matveenko, L.I., et al.
(author)
-
Decimeter-wavelength structure in the quasar 3C 345
- 1986
-
In: Pis'ma v Astronomicheskii Zhurnal. - Moscow : Izdatel'stvo Nauka. - 0320-0108. ; 12:1, s. 63-67
-
Journal article (peer-reviewed)abstract
- The nuclear structure of the quasar 3C 345 has been surveyed at wavelength = 18 and 49 cm with two different VLBI networks. From the nucleus issues a jet, bending as it advances outward. Individual structure components are identified; their radio continuum and that of the nucleus indicate an optically thick source, the break in the spectrum shifting toward lower frequencies with increasing distance from the nucleus.
|
|
| 4. |
- Matveenko, L. I., et al.
(author)
-
The structure of the quasar 3C-345
- 1992
-
In: Soviet Astronomy Letters. - Moscow : Rossijskaja akademija nauk / Russian Academy of Sciences. - 0320-0108. ; 18:6, s. 379-391
-
Journal article (peer-reviewed)abstract
- We study the fine structure of the quasar 3C 345 at a wavelength of 49 cm. The apparent size of the core and low-frequency variability are due to the opacity of the surrounding ionized medium and the electron density distribution. We find the distance dependence of the size and brightness temperature of the components. Relativistic plasma is being ejected into a cone, with vertex angle approximately 40-degrees in position -110-degrees. The jet consists of narrow twisted filaments.
|
|
