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相关论文: A Structure for Quasars

200 篇论文

The origin of the broad emission line region (BELR) in quasars and active galactic nuclei is still unclear. I propose that condensations form in the warm, radiation pressure driven, accretion disk wind of quasars creating the BEL clouds and…

星系天体物理 · 物理学 2017-10-04 Martin Elvis

Quasars are notable for the luminous power they emit across decades in frequency from the far-infrared through hard X-rays; emission at different frequencies emerges from physical scales ranging from AUs to parsecs. Each wavelength regime…

天体物理学 · 物理学 2007-05-23 S. C. Gallagher , J. E. Everett

We investigated a scenario where the presence of a broad absorption line (BAL) feature in quasars (QSOs) is contingent upon the line of sight being situated within an outflow cone emanating from the source. We examined the mechanism of…

星系天体物理 · 物理学 2024-11-20 M. Sniegowska , M. H. Naddaf , M. L. Martinez-Aldama , P. Marziani , S. Panda , B. Czerny

Blue-shifted Broad Absorption Lines (BALs) detected in quasar's spectra are indicative of AGN outflows. We show, using 2D hydrodynamical simulations, that disruption of interstellar clouds by a fast AGN wind can lead to formation of cold,…

高能天体物理现象 · 物理学 2020-01-08 Meir Zeilig Hess , Amir Levinson , Xinfeng Xu , Nahum Arav

We present a unification model for a clumpy obscurer in active galactic nuclei (AGN) and investigate the properties of the resulting X-ray spectrum. Our model is constructed to reproduce the column density distribution of the AGN population…

高能天体物理现象 · 物理学 2019-09-04 Johannes Buchner , Murray Brightman , Kirpal Nandra , Robert Nikutta , Franz E. Bauer

We present the results of X-ray spectral analysis of two mini-BAL QSOs, PG 1126-041 and PG 1351+640, aimed at getting insights into the physics of quasar outflows. We find strong X-ray spectral variability on timescales of years. These…

宇宙学与河外天体物理 · 物理学 2009-12-02 M. Giustini , M. Cappi , G. Chartas , M. Eracleous , G. G. C. Palumbo , C. Vignali

The X-ray weakness of broad absorption line (BAL) quasars in comparison to non-BAL objects is possibly caused by the absorption of X-ray emission by the shielding material near the equatorial plane. On the other hand, the radio-loud BALQSOs…

星系天体物理 · 物理学 2015-06-23 M. Kunert-Bajraszewska , K. Katarzynski , A. Janiuk

Low-ionization broad absorption line (BAL) QSOs present properties that cannot generally be explained by simple orientation effects. We have conducted a deep spectroscopic and imaging study of the host galaxies of the only four BAL QSOs…

天体物理学 · 物理学 2007-05-23 Gabriela Canalizo , Alan Stockton

A new generation of sensitive X-ray measurements are indicating that the existence of X-ray attenuation column densities, $N_{H}>10^{24}\mathrm{cm}^{-2}$ is quite common amongst broad absorption line quasars (BALQSOs). This is significant…

天体物理学 · 物理学 2007-05-23 Brian Punsly , Sebastian Lipari

We present a unification model based on the well-known but mysterious cubic-structure grouping of quarks and leptons that suggests an underlying symmetry connection deemed explainable by a unified theory. It results in an extension of the…

高能物理 - 唯象学 · 物理学 2023-03-13 Mohammad Mehrafarin

We present new integral field spectroscopy of the gravitationally lensed broad absorption line (BAL) quasar H1413+117, covering the ultraviolet to visible rest-frame spectral range. We observe strong microlensing signatures in lensed image…

星系天体物理 · 物理学 2015-11-04 Matthew J. O'Dowd , Nicholas F. Bate , Rachel L. Webster , Kathleen Labrie , Joshua Rogers

We present an algebraic approach to the internal structure of baryons in terms of three constituents. We investigate a collective model in which the nucleon is regarded as a rotating and vibrating oblate top with a prescribed distribution…

核理论 · 物理学 2007-05-23 A. Leviatan , R. Bijker

This review describes recent developments related to the unified model of active galactic nuclei (AGN). It focuses on new ideas about the origin and properties of the central obscurer (torus), and the connection with its surrounding. The…

星系天体物理 · 物理学 2015-09-23 Hagai Netzer

We present new more sensitive high-resolution radio observations of a compact broad absorption line (BAL) quasar, 1045+352, made with the EVN+MERLIN at 5 GHz. They allowed us to trace the connection between the arcsecond structure and the…

宇宙学与河外天体物理 · 物理学 2015-05-19 Magdalena Kunert-Bajraszewska , Agnieszka Janiuk , Marcin P. Gawronski , Aneta Siemiginowska

Broad absorption line quasars are among the objects presenting the fastest outflows. The launching mechanism itself is not completely understood. Models in which they could be launched from the accretion disk, and then curved and…

星系天体物理 · 物理学 2017-07-12 G. Bruni , K. -H. Mack , F. M. Montenegro-Montes , M. Brienza , J. I. González-Serrano

We have used the VLBA at 15 GHz to image the structure of 132 strong compact AGN and quasars with a resolution better than one milliarcsecond and a dynamic range typically exceeding 1000 to 1. These observations were made as part of a…

天体物理学 · 物理学 2009-10-30 K. I. Kellermann , R. C. Vermeulen , J. A. Zensus , M. H. Cohen

If broad absorption line (BAL) quasars represent a high covering fraction evolutionary state (even if this is not the sole factor governing the presence of BALs), it is expected that they should show an excess of mid-infrared radiation…

宇宙学与河外天体物理 · 物理学 2015-06-12 M. A. DiPompeo , J. C. Runnoe , M. S. Brotherton , A. D. Myers

The various ionization mechanisms at play in active galactic nuclei (AGN) and quasars have been well studied, but relatively little has been done to separately investigate the contributions of these ionization mechanisms within the host…

星系天体物理 · 物理学 2019-08-14 Jason T. Hinkle , Sylvain Veilleux , David S. N. Rupke

In this paper, we report the line-locking phenomenon of the blended narrow absorption lines (NALs) within trough-like broad absorption lines (BALs) in quasar SDSS J021740.96--085447.9 (hereafter J0217--0854). Utilizing the two-epoch…

星系天体物理 · 物理学 2018-08-29 Wei-Jian Lu , Ying-Ru Lin

This talk discusses the unified X-ray/UV absorption models in AGN. I will first review the models and discuss how they offer an unique opportunity to probe the near nuclear environment of AGNs. Recently, however, the validity of these…

天体物理学 · 物理学 2007-05-23 Smita Mathur