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We present a sample of 28 objects at z<0.3 from Data Release 16 of the Sloan Digital Sky Survey (SDSS DR16) with large velocity offset (> 200 km/s) of narrow H$\beta$ and H$\alpha$ emission lines relative to absorption lines. Diagnostic…

星系天体物理 · 物理学 2025-11-18 Zheng Qi , Zhang Xueguang , Yuan Qirong

We report on the study of an intriguing active galaxy that was selected as a potential multiple supermassive black hole merger in the early-type host SDSS J151709.20+335324.7 (z=0.135). Ground-based SDSS imaging reveals two blue structures…

宇宙学与河外天体物理 · 物理学 2015-05-18 D. J. Rosario , G. A. Shields , G. B. Taylor , S. Salviander , K. L. Smith

We report Chandra observations of a double X-ray source in the z=0.1569 galaxy SDSS J171544.05+600835.7. The galaxy was initially identified as a dual AGN candidate based on the double-peaked [O III] emission lines, with a line-of-sight…

宇宙学与河外天体物理 · 物理学 2012-06-19 Julia M. Comerford , David Pooley , Brian F. Gerke , Greg M. Madejski

In this paper, we presented a detailed analysis of the Sloan Digital Sky Survey optical spectrum of a new sub-kpc scale dual AGN candidate SDSS J222428.53+261423.2 (=SDSS J2224). The target is one of the few AGNs with all the optical narrow…

星系天体物理 · 物理学 2024-04-22 Qi Zheng , XueGuang Zhang , QiRong Yuan , Paola Severgnini , Cristian Vignali

The quasar SDSS J153636.22+044127.0, exhibiting peculiar broad emission-line profiles with multiple components, was proposed as a candidate sub-parsec binary supermassive black hole system. More recently, imaging revealed two spatially…

宇宙学与河外天体物理 · 物理学 2015-05-13 Ryan Chornock , J. S. Bloom , S. B. Cenko , A. V. Filippenko , J. M. Silverman , M. D. Hicks , K. J. Lawrence , A. J. Mendez , M. Rafelski , A. M. Wolfe , ;

We analyze the optical spectrum of type 1 QSO SDSS J1425+3231. This ob- ject is interesting since its narrow emission lines such as [O III]{\lambda}{\lambda}4959, 5007 are double- peaked, and the line structure can be modeled well by three…

宇宙学与河外天体物理 · 物理学 2015-05-20 Zhixin Peng , Yanmei Chen , Qiusheng Gu , Chen Hu

In the manuscript, a candidate of sub-pc binary black hole (BBH) system is reported in SDSS J1257+2023 through different properties of broad Balmer emission lines. After subtractions of host galaxy contributions, Gaussian functions are…

星系天体物理 · 物理学 2023-08-02 XueGuang Zhang

In the HST/COS spectrum of the Seyfert 1 galaxy 2MASX J14292507+4518318, we have identified a narrow absorption line (NAL) outflow system with a velocity of -151 km s$^{-1}$ This outflow exhibits absorption troughs from the resonance states…

星系天体物理 · 物理学 2023-11-30 Maryam Dehghanian , Nahum Arav , Doyee Byun , Gwen Walker , Mayank Sharma

We present an analysis of the active galaxy SDSS J131642.90+175332.5, which is remarkable because all of its narrow emission lines are double-peaked, and because it additionally shows an extra broad component (FHWM ~ 1400 km/s) in most of…

星系天体物理 · 物理学 2015-05-14 Dawei Xu , S. Komossa

Most massive galaxies contain supermassive black holes (SMBHs) in their cores. When galaxies merge, gas is driven to nuclear regions and can accrete onto the central black hole. Thus one expects to see dual AGN in a fraction of galaxy…

宇宙学与河外天体物理 · 物理学 2015-05-28 R. C. McGurk , C. E. Max , D. J. Rosario , G. A. Shields , K. L. Smith , S. A. Wright

We obtained Keck/OSIRIS near-IR adaptive optics-assisted integral-field spectroscopy to probe the morphology and kinematics of the ionized gas in four velocity-offset active galactic nuclei (AGNs) from the Sloan Digital Sky Survey. These…

星系天体物理 · 物理学 2016-10-19 Francisco Müller-Sánchez , Julia M. Comerford , Daniel Stern , Fiona A. Harrison

In this manuscript, an interesting method is proposed to test dual core system for double-peaked narrow emission lines, through precious dual core system with double-peaked narrow Balmer lines in one system in main galaxy but with…

星系天体物理 · 物理学 2023-02-06 Zhang XueGuang , Zheng Qi

We present a study of the radial velocity offsets between narrow emission lines and host galaxy lines (stellar absorption and H I 21-cm emission) in Seyfert galaxies with observed redshifts less than 0.043. We find that 35% of the Seyferts…

宇宙学与河外天体物理 · 物理学 2014-11-20 D. M. Crenshaw , H. R. Schmitt , S. B. Kraemer , R. F. Mushotzky , J. P. Dunn

Double-peaked Balmer lines have been observed in about 150 AGNs and were interpreted preferably as emission from relativistic accretion disks. In this paper, we report the discovery of extreme double-peaked lines in SDSS J0942+0900 and SDSS…

天体物理学 · 物理学 2009-11-11 T. G. Wang , X. B. Dong , X. G. Zhang , H. Y. Zhou , J. X. Wang , Y. J. Lu

In this letter, we report the discovery of a fast neutral hydrogen outflow in SDSS J145239.38+062738.0, a merging radio galaxy containing an optical type I active galactic nuclei (AGN). This discovery was made through observations conducted…

We identify SDSS J153636.22+044127.0, a QSO discovered in the Sloan Digital Sky Survey, as a promising candidate for a binary black hole system. This QSO has two broad-line emission systems separated by 3500 km/sec. The redder system at…

星系天体物理 · 物理学 2009-11-13 Todd A. Boroson , Tod R. Lauer

SDSSJ092712.65+294344.0 was identified by the SDSS as a quasar, but has the unusual property of having two emission line systems offset by 2650 km/s. One of these contains the usual combination of broad and narrow lines, the other only…

天体物理学 · 物理学 2011-02-11 Timothy M. Heckman , Julian H. Krolik , Sean M. Moran , Jeremy Schnittman , Suvi Gezari

With the aim of investigating galaxies with two strong simultaneous starbursts, we have extracted a sample of galaxies with double-peaked emission lines in their global spectra from the SDSS spectral database. We then fitted the emission…

宇宙学与河外天体物理 · 物理学 2015-05-30 L. S. Pilyugin , I. A. Zinchenko , B. Cedres , J. Cepa , A. Bongiovanni , L. Mattsson , J. M. Vilchez

While 2% of active galactic nuclei (AGNs) exhibit narrow emission lines with line-of-sight velocities that are significantly offset from the velocity of the host galaxy's stars, the nature of these velocity offsets is unknown. We…

星系天体物理 · 物理学 2017-10-04 Julia M. Comerford , R. Scott Barrows , Jenny E. Greene , David Pooley

The quasar SDSS J105041.35+345631.3 (z = 0.272) has broad emission lines blueshifted by 3500 km/s relative to the narrow lines and the host galaxy. Such an object may be a candidate for a recoiling supermassive black hole, binary black…

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