Zobrazeno 1 - 10
of 36
pro vyhledávání: '"J. J. Puschell"'
Publikováno v:
Extragalactic Radio Sources ISBN: 9789400977839
Extragalactic Radio Sources ISBN: 9789401175678
Extragalactic Radio Sources ISBN: 9789401175678
Calculations modeling the effects of stellar evolution on elliptical galaxies (e.g., Bruzual and Kron 1980, Bruzual 1981) suggest that the shape of the spectral flux distribution should remain almost constant in the red and near-infrared out to at le
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3724a1ccaa1bb17a9b35c2a897d4fc4f
https://doi.org/10.1007/978-94-009-7781-5_117
https://doi.org/10.1007/978-94-009-7781-5_117
Publikováno v:
Early Evolution of the Universe and its Present Structure ISBN: 9789027716620
This paper is concerned with the distant radio galaxies in a sample of bright sources selected at 178 MHz by Laing, Riley & Longair (1982). This sample is 96% complete for sources with θ 20, using the VIA at a wavelength of 6 cm (Laing, Owen & Pusch
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::42f5d4a5d6fbaaf881935bfc9b3263b0
https://doi.org/10.1007/978-94-009-7220-9_20
https://doi.org/10.1007/978-94-009-7220-9_20
Publikováno v:
Extragalactic Radio Sources ISBN: 9789400977839
Extragalactic Radio Sources ISBN: 9789401175678
Extragalactic Radio Sources ISBN: 9789401175678
The purpose of this communication is to update our knowledge of the radio structural properties of quasars and blank field radio sources (blank field ≡ any radio source without an identification on the Palomar Sky Survey prints). The quasar sample
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2e1ffc1cfbbdc507de524f66274d0d39
https://doi.org/10.1007/978-94-009-7781-5_121
https://doi.org/10.1007/978-94-009-7781-5_121
Autor:
Robert Landau, Thomas J. Balonek, Eugene E. Epstein, Thomas W Jones, Michael W. Werner, G. Neugebauer, J. J. Puschell, B. T. Soifer
Observations simultaneously made at visual (B, V, and R) wavelengths, at 1, 1.4, and 3.4 mm and at 1.3, 2, 6, and 20 cm of 9 QSOs and BL Lac objects are reported. The range of the millimeter visual spectral index ɑ_(mv) was only 0.65-0.82, typical o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d772b43458ab5780ae52fdb83ec7660
https://resolver.caltech.edu/CaltechAUTHORS:20140319-131640084
https://resolver.caltech.edu/CaltechAUTHORS:20140319-131640084
Publikováno v:
Astrophysical Journal
Astrophysical Journal, 285, 515-526
Astrophysical Journal, 285, 515-526
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c591619a93e014aa7e9afd8666a7cc65
https://hdl.handle.net/1887/6467
https://hdl.handle.net/1887/6467
Publikováno v:
Symposium - International Astronomical Union. 97:423-424
Calculations modeling the effects of stellar evolution on elliptical galaxies (e.g., Bruzual and Kron 1980, Bruzual 1981) suggest that the shape of the spectral flux distribution should remain almost constant in the red and near-infrared out to at le
Publikováno v:
Nature. 283:357-358
In a search for radio emission from bright, optically selected quasars, we detected ∼50% of the quasars at 5 GHz. This radio detection rate is so much higher than that for faint quasars (
Publikováno v:
Symposium - International Astronomical Union. 104:85-86
This paper is concerned with the distant radio galaxies in a sample of bright sources selected at 178 MHz by Laing, Riley & Longair (1982). This sample is 96% complete for sources with θ < 10′ and the bias of the 3CR catalogue against sources of l
Publikováno v:
Symposium - International Astronomical Union. 97:435-436
The purpose of this communication is to update our knowledge of the radio structural properties of quasars and blank field radio sources (blank field ≡ any radio source without an identification on the Palomar Sky Survey prints). The quasar sample
Publikováno v:
The Astrophysical Journal. 303:L37
1200-3200 A IUE spectra of the nucleus of NGC 4552 (M89) were obtained in order to investigate the nature of the strong 10 micron source in this Galaxy. There is a strong, extended UV source in NGC 4552 which has a spatial distribution nearly identic