1993
DOI: 10.1093/mnras/264.2.298
|View full text |Cite
|
Sign up to set email alerts
|

VLA observations of a complete sample of core-dominated radio sources

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

10
187
1
1

Year Published

1996
1996
2016
2016

Publication Types

Select...
7
1

Relationship

0
8

Authors

Journals

citations
Cited by 181 publications
(203 citation statements)
references
References 0 publications
10
187
1
1
Order By: Relevance
“…It has been extensively studied in the past at different radio wavelengths. At kpc scales, the maps reveal components south of the core at 2, 37, and 45 arcsec (Antonucci et al 1986;Strom & Biermann 1991;Murphy et al 1993). Eckart et al (1987) and Pearson & Readhead (1988) reported a core-jet structure at pc scales with a jet oriented westwards.…”
Section: Bl 1803+784mentioning
confidence: 92%
See 1 more Smart Citation
“…It has been extensively studied in the past at different radio wavelengths. At kpc scales, the maps reveal components south of the core at 2, 37, and 45 arcsec (Antonucci et al 1986;Strom & Biermann 1991;Murphy et al 1993). Eckart et al (1987) and Pearson & Readhead (1988) reported a core-jet structure at pc scales with a jet oriented westwards.…”
Section: Bl 1803+784mentioning
confidence: 92%
“…Its radio structure has been studied at pc and kpc scales by Appl et al (1996), who reported a misalignment of the jet between both scales. At kpc scales, Murphy et al (1993) reported a VLA map with a core and a fainter component at 6 arcsec and PA ∼ −100 • . At pc scales, Eckart et al (1987) reported a core-jet structure in the VLBI maps, with a faint jet emission oriented at .93) and 28 May 1999(1999.…”
Section: Qso 1150+812mentioning
confidence: 99%
“…Except for that, there is a significant decrease in the flux density at 408 MHz, suggesting a low frequency turnover around 1 GHz in the spectrum. The Very Large Array (VLA) observation performed at 1.5 GHz in 1984 revealed a bright compact component and a weak feature about 4.9 ′′ to the southwest (Murphy et al, 1993).…”
Section: Cso Identification Of 2234+282mentioning
confidence: 99%
“…This is a misaligned source, with its VLA jet at almost 90 degrees position angle to the Very Long Baseline Array (VLBA) jet (Murphy et al 1993;Britzen et al 2007). A jet in the western direction with a sharp bend to the south at about 50 mas was detected by Polatidis et al (1995) observations at 5 GHz (Barthel et al 1995).…”
Section: Introductionmentioning
confidence: 89%