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It is shown that there are at least 21 QSOs within 1 degree of the nearby active spiral galaxy NGC3079. Many of them are bright (mag<18) so that the surface density of those closer than 15 arc minutes to the galaxy centre is close to 100…

天体物理学 · 物理学 2007-05-23 E. M. Burbidge , G. Burbidge , H. C. Arp , W. M. Napier

A panchromatic view of the star forming ring and feeding process in the central kpc of the galaxy NGC 1097 is presented. The assembled IR to UV images at $\sim$10 pc resolution allow us to characterise the population of circa 250 clusters…

Observations with the Wide-Field Camera of the Hubble Space Telescope are presented for a representative sample of 20 intrinsically luminous quasars with redshifts smaller than 0.30. These observations show that luminous quasars occur in…

天体物理学 · 物理学 2011-07-18 John N. Bahcall , Sofia Kirhakos , David H. Saxe , Donald P. Schneider

Very deep imaging data of three optically luminous radio-loud quasars with redshifts between z=0.9 and z=1.36 are presented. The data are complete for galaxies down to R=26. There is no evidence for excess numbers of galaxies around the…

天体物理学 · 物理学 2007-05-23 J. W. Fried

We present $B,V,R,J,H,K$ broad--band images of the barred galaxy NGC 1097. The optical and infrared colors maps trace the location of the major dust features. The dust lanes are relatively free of star formation and have low opacity. The…

天体物理学 · 物理学 2009-10-28 A. C. Quillen , Jay. A. Frogel , L. E. Kuchinski , D. M. Terndrup

NGC 3079 is a very active, disturbed galaxy which has been observed to have X-ray and radio ejections from it as well as an optical superbubble along its minor axis. Here we show that the brightest X-ray sources within about 40 arcmin are…

天体物理学 · 物理学 2007-05-23 H. Arp , E. M. Burbidge

There is controversy about the measurement of statistical associations between bright quasars and faint, presumably foreground galaxies. We look at the distribution of galaxies around an unbiased sample of 63 bright, moderate redshift…

天体物理学 · 物理学 2015-06-24 P. A. Thomas , R. L. Webster , M. J. Drinkwater

The circumnuclear star-forming ring of the barred spiral galaxy NGC 1097 provides a unique laboratory to study star formation under extreme conditions. This work aims to derive the physical properties of the circumnuclear star-forming…

星系天体物理 · 物理学 2026-02-11 Sandra Zamora , Angeles I. Díaz , Asier Castrillo

The detection of resonance absorption lines against known objects such as individual galaxies and clusters of galaxies is a powerful approach for studying the gas content of these systems. We describe an efficient method of identifying…

天体物理学 · 物理学 2009-10-30 Patricia M. Knezek , Joel N. Bregman

We have conducted ultra-deep optical and deep near-infrared observations of a field around the z=1.226 radio-quiet quasar 104420.8+055739 from the Clowes-Campusano LQG of 18 quasars at z~1.3 in search of associated galaxy clustering.…

天体物理学 · 物理学 2015-06-24 C. P. Haines , R. G. Clowes , L. E. Campusano , A. J. Adamson

UGC 8584 was selected by a computer program as having a number of quasars around it that obeyed the Karlsson periodicity in its reference frame. On closer examination 9 of the nearest 10 quasars turned out to be extremely close to the…

天体物理学 · 物理学 2008-03-19 H. Arp , C. Fulton

This review attempts to describe developments in the fields of quasar and quasar host galaxies in the past five. In this time period, the Sloan and 2dF quasar surveys have added several tens of thousands of quasars, with Sloan quasars being…

天体物理学 · 物理学 2015-06-24 Mark Lacy

Quasars behind the Galactic plane (GPQs) are important astrometric references and valuable probes of Galactic gas, yet the search for GPQs is difficult due to severe extinction and source crowding in the Galactic plane. In this paper, we…

During analysis of the relation of quasars to galaxies in the 2dF deep field a concentration of quasars was noted. Most striking was the closeness in redshift of 14 quasars about the mean redshift z = 2.149 with a range of $\pm 0.018$. The…

天体物理学 · 物理学 2008-02-13 H. Arp , C. Fulton

We present an investigation of the environment (\approx 600 kpc radius) of a pair of luminous z=4.25 quasars, SDSS J1439-0034 A,B, separated by 33''. An analysis of high-quality Subaru spectra of the quasars suggests that this configuration…

天体物理学 · 物理学 2009-11-10 Masataka Fukugita , Osamu Nakamura , Donald P. Schneider , Mamoru Doi , Nobunari Kashikawa

We present a sample of quasars discovered in the area of Galactic Anti-Center (GAC) of $150^{\circ} \leq l \leq 210^{\circ}$ and $|b| \leq 30^{\circ}$, based on the LAMOST Data Release 3 (DR3). The sample contains 151 spectroscopically…

The central kpc region of the low luminosity type-1 Seyfert galaxy NGC 1097 has been observed in the CO(1-0) and HCN(1-0) lines with the Nobeyama Millimeter Array and the NRO 45 m telescope. We find a striking enhancement of the HCN…

天体物理学 · 物理学 2015-06-24 K. Kohno , S. Ishizuki , S. Matsushita , B. Vila-Vilaro , R. Kawabe

We present deep imaging and spectroscopic observations of the z = 1.195 quasar 3C 190 and its immediate environment. The quasar is surrounded by an asymmetric low-surface-brightness envelope in which there are also several galaxies with…

天体物理学 · 物理学 2009-11-06 Alan Stockton , Susan E. Ridgway

We report the discovery of 40 bright quasars and active galactic nuclei (AGNs) at low Galactic latitude (b<20deg). The low Galactic latitude region has been considered a place to avoid when searching for extragalactic sources, because of…

天体物理学 · 物理学 2009-06-23 Myungshin Im , Induk Lee , Yunseok Cho , Changsu Choi , Jongwan Ko , Mimi Song

We obtained medium-resolution spectra of 336 quasar candidates in the COSMOS HST/Treasury field using the MMT 6.5-meter telescope and the Hectospec multi-object spectrograph. Candidates were drawn from the Sloan Digital Sky Survey (SDSS)…

天体物理学 · 物理学 2009-11-11 M. K. M. Prescott , C. D. Impey , R. J. Cool , N. Z. Scoville
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