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相关论文: Polarimetry and Unification of Low-Redshift Radio …

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We present optical spectropolarimetric and imaging polarimetric observations of four high-redshift radio galaxies (HzRGs) obtained with the 10-m Keck I telescope. A broad Mg II emission line is detected in the total and polarized flux…

Polarimetry of the narrow-line radio galaxy PKS 0116+082 at the W.M. Keck telescope shows that it has high and variable optical polarization, presumably due to synchrotron radiation. It is not a BL Lac object because it has strong narrow…

天体物理学 · 物理学 2009-10-30 M. H. Cohen , R. C. Vermeulen , P. M. Ogle , H. D. Tran , R. W. Goodrich

Radio galaxies are linearly polarized -- an important property that allows us to infer the properties of the magnetic field of the source and its environment. However at low frequencies, Faraday rotation substantially depolarizes the…

We present the results of spectropolarimetry of a sample of 7 powerful radio galaxies and 2 quasars with $0.07<z<0.35$ obtained to detect possible anisotropies in the [OIII] line emission, which could explain the higher [OIII] luminosity of…

天体物理学 · 物理学 2007-05-23 Sperello di Serego Alighieri , Andrea Cimatti , R. A. E. Fosbury , Ronald Hes

We have carried out a spectropolarimetric search for hidden broad-line quasars in three ultraluminous infrared galaxies (ULIRGs) discovered in the positional correlations between sources detected in deep radio surveys and the IRAS Faint…

天体物理学 · 物理学 2009-10-31 Hien D. Tran , M. S. Brotherton , S. A. Stanford , Wil van Breugel , A. Dey , D. Stern , R. Antonucci

With high-sensitivity kiloparsec-scale radio polarimetry, we can examine the jet-medium interactions and get a better understanding of the blazar divide in radio-loud (RL) AGN. We are analyzing the radio polarimetric observations with the…

星系天体物理 · 物理学 2023-04-25 Janhavi Baghel , P. Kharb , Silpa S. , Luis C. Ho , C. M. Harrison

We present the results of UV spectropolarimetry (2000 - 3000A) and far-UV spectroscopy (1500 - 2000A) of two low-redshift narrow-line radio galaxies (NLRGs) taken with the Faint Object Spectrograph onboard the Hubble Space Telescope (HST).…

In the unified schemes for extragalactic radio sources, the quasars and BL Lac objects are intrinsically similar to the Fanaroff-Riley class II and I radio galaxies respectively, but appear to be different because they are viewed at…

天体物理学 · 物理学 2009-10-31 D. J. Saikia

We present deep radio images at 1.4 GHz of a large and complete sample of BL Lacertae objects (BL Lacs) selected from the Deep X-ray Radio Blazar Survey (DXRBS). We have observed 24 northern sources with the Very Large Array (VLA) in both…

天体物理学 · 物理学 2009-11-13 Hermine Landt , Hayley E. Bignall

We present new spectropolarimetric observations of 8 radio-loud broad absorption line (BAL) quasars, and combine these new data with our previous spectropolarimetric atlases (of both radio-loud and radio-quiet objects) in order to…

宇宙学与河外天体物理 · 物理学 2015-06-11 M. A. DiPompeo , M. S. Brotherton , C. De Breuck

We present an analysis of 2.05 $\mu$m Hubble Space Telescope (HST) polarimetric data for a sample of 13 nearby Fanaroff-Riley type II (FRII) 3CR radio sources ($0.03<z<0.11$) that are classified as narrow line radio galaxies (NLRG) at…

星系天体物理 · 物理学 2015-06-22 E. A. Ramírez , C. N. Tadhunter , D. Axon , D. Batcheldor , C. Packham , E. Lopez-Rodriguez , W. Sparks , S. Young

We report spectropolarimetry of 30 radio-selected broad absorption line (BAL) quasars with the Keck Observatory, 25 from the sample of Becker et al. (2000). Both high and low-ionization BAL quasars are represented, with redshifts ranging…

宇宙学与河外天体物理 · 物理学 2015-05-19 M. A. DiPompeo , M. S. Brotherton , R. H. Becker , H. D. Tran , M. D. Gregg , R. L. White , S. A. Laurent-Muehleisen

In order to determine whether unified models of active galactic nuclei apply to low-luminosity objects, we have undertaken a spectropolarimetric survey of of LINERs and Seyfert nuclei at the Keck Observatory. The 14 objects observed have a…

天体物理学 · 物理学 2009-10-31 A. J. Barth , A. V. Filippenko , E. C. Moran

Updates are provided on several issues related to Unified Models. A new HST spectrum of Cygnus A confirms the broad MgII emission line, and suggests a very large velocity width as seen in the polarized optical lines. Statistics of the 3CR…

天体物理学 · 物理学 2007-05-23 Robert Antonucci

We address the nature of broad-lined radio galaxies, in particular their radio axis orientation, using new, matched resolution, dual frequency radio observations of a sample of twelve nearby broad-lined extragalactic 3C objects. Radio…

天体物理学 · 物理学 2007-05-23 J. Dennett-Thorpe , P. D. Barthel , I. M. van Bemmel

This paper concerns the relationship of BLLacs and flat spectrum weak emission-line galaxies. We compare the weak emission-line galaxies and the BLLacs in a sample of 57 flat spectrum objects (Marcha et al. 1996), using high-frequency radio…

天体物理学 · 物理学 2007-05-23 J. Dennett-Thorpe , M. J. Marcha

We have observed seven powerful FR2 radiogalaxies and seven quasars with the Spitzer IRS. Both samples are comparable in both, redshift range and isotropic 178 Hz luminosity. Both samples are found to have similar distributions in the…

天体物理学 · 物理学 2007-05-23 Bernhard Schulz , Ralf Siebenmorgen , Martin Haas , Endrik Kruegel , Rolf Chini

We present the soft X-ray (0.1--2.4 keV) properties of a complete sample of 88 southern radio sources derived from the Wall \& Peacock 2-Jy sample. It comprises 68 radio galaxies, 18 quasars and 2 BL Lac objects. Whereas both BL Lac objects…

With the Spitzer Space Telescope Infrared Spectrograph (IRS) we have observed seven powerful FR2 radio galaxies and seven quasars. Both samples, the galaxies and the quasars, are comparable in isotropic 178 MHz luminosity (10^26.5 W/Hz < P…

天体物理学 · 物理学 2009-11-11 Martin Haas , Ralf Siebenmorgen , Bernhard Schulz , Endrik Kruegel , Rolf Chini

We present new spectroscopic identifications for 169 objects in the RASS-Green Bank (RGB) catalog of radio- and X-ray-emitting AGN. These data significantly increase the fraction of bright RGB objects with classifications. Specifically, we…

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