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相关论文: Light-year Scale Radio Cores in Four LINER Galaxie…

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A VLA survey of nearby LINER galaxies at 15 GHz has revealed the presence of a compact radio core in many sources. The cores seem to be correlated with the optical activity. Follow-up VLBA observations of the ten brightest sources confirm…

天体物理学 · 物理学 2007-05-23 Heino Falcke , Luis C. Ho , James S. Ulvestad , Andrew S. Wilson , Neil M. Nagar

The low-luminosity active galactic nuclei in NGC 3147, NGC 4203, and NGC 4579 have been imaged at four frequencies with the Very Long Baseline Array. The galaxies are unresolved at all frequencies, with size upper limits of $10^3-10^4$…

天体物理学 · 物理学 2009-11-07 James S. Ulvestad , Luis C. Ho

(abbreviated): This paper presents the results of a high resolution radio imaging survey of all known (96) low-luminosity active galactic nuclei (LLAGNs) at D<19Mpc. We find that almost half of all LINERs and low-luminosity Seyferts have…

天体物理学 · 物理学 2009-11-07 N. M. Nagar , H. Falcke , A. S. Wilson , J. S. Ulvestad

We present preliminary results of a study of the low frequency radio continuum emission from the nuclei of Giant Low Surface Brightness (LSB) galaxies. We have mapped the emission and searched for extended features such as radio lobes/jets…

天体物理学 · 物理学 2009-11-13 M. Das , S. S. McGaugh , N. Kantharia , S. N. Vogel

In this letter, we report on dual-frequency European VLBI Network (EVN) observations of the faintest and least luminous radio cores in Seyfert nuclei, going to sub-mJy flux densities and radio luminosities around 10^19 W/Hz. We detect radio…

宇宙学与河外天体物理 · 物理学 2014-11-20 Marcello Giroletti , Francesca Panessa

We report the results of high-resolution 5 GHz Very Long Baseline Array and European VLBI Network observations of 36 nearby galaxies, an extension of the Legacy e-MERLIN Multi-band Imaging of Nearby Galaxies (LeMMINGs) survey. Our sample…

In this paper we present the results of VLBI observations of six radio galaxies belonging to the 2-Jy sample. The selected objects are 3C17, PKS 0620-52, PKS 0625-35, PKS 1318-43, PKS 1333-33 and 3C317. The first is a high power radio…

天体物理学 · 物理学 2007-05-23 T. Venturi , R. Morganti , T. Tzioumis , J. Reynolds

We report on sensitive dual-frequency (1.7 and 5 GHz) European VLBI Network observations of the central region of nine Seyfert galaxies. These sources are among the faintest and least luminous members of a complete sample of nearby (d<22…

宇宙学与河外天体物理 · 物理学 2015-06-11 P. Bontempi , M. Giroletti , F. Panessa , M. Orienti , A. Doi

We report a 0.2" resolution, 15 GHz survey of a sample of 48 low-luminosity active galactic nuclei with the Very Large Array. Compact radio emission has been detected in 57% (17 of 30) of LINERs and low-luminosity Seyferts, at least 15 of…

天体物理学 · 物理学 2009-10-31 Neil M. Nagar , Heino Falcke , Andrew S. Wilson , Luis C. Ho

The results of Chandra snapshot observations of 11 LINERs (Low-Ionization Nuclear Emission-line Regions), three low-luminosity Seyfert galaxies, and one HII-LINER transition object are presented. Our sample consists of all the objects with…

天体物理学 · 物理学 2007-05-23 Yuichi Terashima , Andrew S. Wilson

According to optical stellar kinematics observations, an over-massive black hole candidate has been reported by van den Bosch et al. (2012) in the normal early-type galaxy NGC 1277. This galaxy is located in the central region of the…

星系天体物理 · 物理学 2017-01-11 Songyoun Park , Jun Yang , J. B. Raymond Oonk , Zsolt Paragi

We present here new VLBI observations of one FR-I radio galaxy (NGC2484) and two Broad Line FR-II radio galaxies (3C109 and 3C382). For 3C109 new VLA maps are also shown. These sources belong to a complete sample of radio galaxies under…

天体物理学 · 物理学 2009-10-22 G. Giovannini , L. Feretti , T. Venturi , L. Lara , J. Marcaide , M. Rioja , S. R. Spangler , A. E. Wehrle

We present new Very Long Baseline Interferometry observations of the LINER galaxy NGC 4278. The observations were taken with the Very Long Baseline Array (VLBA) and a single antenna of the Very Large Array (VLA) at 5 GHz and 8.4 GHz and…

天体物理学 · 物理学 2015-06-24 M. Giroletti , G. B. Taylor , G. Giovannini

High resolution MERLIN 5 GHz observations (0.04") of 7 Seyfert galaxies, selected as the ones previously showing evidence of collimated ejection, have been compared with high resolution archive HST data. The radio maps reveal rich…

天体物理学 · 物理学 2009-11-11 E. Xanthopoulos , A. H. Thean , A. Pedlar , A. M. S. Richards

LINERs exist in the nuclei of a large fraction of luminous galaxies, but their connection with the AGN phenomenon has remained elusive. We present Hubble Space Telescope narrowband [O III]5007 and H-alpha+[N II] emission-line images of the…

天体物理学 · 物理学 2009-10-31 R. W. Pogge , D. Maoz , L. C. Ho , M. Eracleous

We present submillimeter continuum observations at 870 microns of the cores of low redshift 3CRR radio galaxies, observed at the Heinrich Hertz Submillimeter Telescope. The cores are nearly flat spectrum between the radio and submillimeter…

天体物理学 · 物理学 2009-11-10 A. C. Quillen , Jessica Almog , Mihoko Yukita

Compact radio cores are not only common in radio galaxies and quasars but also in many nearby galaxies with low-active, supermassive black holes. One famous example is the Galactic Center source Sgr A*. Recent studies of proper motions and…

天体物理学 · 物理学 2007-05-23 Heino Falcke

We have used the VLBA at 5 GHz to observe all galaxies with nuclear radio flux densities above 3.5 mJy found in a VLA survey at 15 GHz of a sample of nearby LINER galaxies. All galaxies were detected revealing high brightness temperature…

天体物理学 · 物理学 2009-10-31 Heino Falcke , Neil M. Nagar , Andrew S. Wilson , James S. Ulvestad

The Seyfert galaxy NGC 4151 has been imaged at resolution better than 0.1 pc using a VLBI array consisting of the VLBA and three 100m-class telescopes. A flat-spectrum 3-mJy source with a monochromatic radio power of ~10^{37} ergs/s has…

天体物理学 · 物理学 2008-11-26 James S. Ulvestad , Diane S. Wong , Gregory B. Taylor , Jack F. Gallimore , Carole G. Mundell

Less than $200$ radio-loud active galactic nuclei (AGN) are known above redshift $4$. Around $40$ of them have been observed at milliarcsecond (mas) scale resolution with very long baseline interferometry (VLBI) technique. Some of them are…

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