Results 1 to 10 of about 758,851 (211)

SDSS-IV MaNGA: How Galaxy Interactions Influence Active Galactic Nuclei

open access: yesThe Astrophysical Journal, 2023
We present a comparative study of active galactic nuclei (AGN) between galaxy pairs and isolated galaxies with the final data release of the MaNGA integral field spectroscopic survey.
Joshua L. Steffen   +9 more
doaj   +1 more source

A Census of WISE-selected Dual and Offset AGNs Across the Sky: New Constraints on Merger-driven Triggering of Obscured AGNs

open access: yesThe Astrophysical Journal, 2023
Pairs of galaxies hosting active galactic nuclei (AGNs) are powerful probes of merger-driven supermassive black hole (SMBH) growth as they can resolve individual AGNs and trace mergers over a large range of physical separations.
R. Scott Barrows   +3 more
doaj   +1 more source

The Effect of Age on the Grouping of Open Clusters: II—Are There Old Binary Clusters?

open access: yesUniverse, 2022
In the present study, we continue testing the Primordial Group hypothesis (Casado 2022), which postulates that only sufficiently young open clusters can be binary or multiple, and old clusters are essentially single.
Juan Casado
doaj   +1 more source

Detection of the Low-stellar-mass Host Galaxy of a z ∼ 6.25 Quasar with JWST

open access: yesThe Astrophysical Journal, 2023
We characterize the stellar mass of J2239+0207, a z ∼ 6.25 sub-Eddington quasar ( M _1450 = −24.6), using dedicated JWST/NIRCam medium-band observations of a nearby point-spread function star to remove the central point source and reveal the underlying ...
Meredith A. Stone   +3 more
doaj   +1 more source

NO THE HOLMBERG EFFECT FOR GALAXY PAIRS SELECTED FROM THE SDSS DR9 AT Z ≤ 0:06

open access: yesOdessa Astronomical Publications, 2016
We studied the Holmberg effect in galaxy pairs selected from the SDSS DR9, where 60561galaxies were limited by redshift 0.02 < z < 0.06 and absolute magnitude: Mr ≤ −20.7 m for central galaxies (N=18578) and Mr > −21.5 m for neighbor galaxies (N=41983 ...
D. V. Dobrycheva, I. B. Vavilova
doaj   +1 more source

A Chandra X-Ray Survey of Optically Selected Close Galaxy Pairs: Unexpectedly Low Occupation of Active Galactic Nuclei

open access: yesThe Astrophysical Journal, 2023
High-resolution X-ray observations offer a unique tool for probing the still-elusive connection between galaxy mergers and active galactic nuclei (AGNs).
Lin He   +4 more
doaj   +1 more source

Sunyaev Zel’dovich high resolution view of filamentary structures between galaxy clusters pairs [PDF]

open access: yesEPJ Web of Conferences, 2022
Strong observational and theoretical evidences suggest that about half of the baryons in the Universe should lie outside galaxy clusters in a lowdensity and hot phase in filaments connecting galaxy clusters.
Radiconi Federico
doaj   +1 more source

Circumgalactic Lyα Nebulae in Overdense Quasar Pair Regions Observed with the Palomar Cosmic Web Imager

open access: yesThe Astrophysical Journal, 2023
The recent discovery of enormous Ly α nebulae (ELANe), characterized by physical extents >200 kpc and Ly α luminosities >10 ^44 erg s ^−1 , provides a unique opportunity to study the intergalactic medium and circumgalactic medium in distant galaxies ...
Jessica S. Li   +10 more
doaj   +1 more source

The Study of the Circumgalactic Medium with Quasar Pairs

open access: yesThe Astrophysical Journal Supplement Series, 2023
We have collected 10,025 foreground–background quasar pairs with projected distances d _p < 500 kpc from the large quasar catalog of the Sloan Digital Sky Survey DR16Q. We investigate the properties of the Mg ii absorption lines with W _r > 0.15 Å around
Zhi-Fu Chen   +7 more
doaj   +1 more source

Statistics of Galactic-scale Quasar Pairs at Cosmic Noon

open access: yesThe Astrophysical Journal, 2023
The statistics of galactic-scale quasar pairs can elucidate our understanding of the dynamical evolution of supermassive black hole (SMBH) pairs, the duty cycles of quasar activity in mergers, or even the nature of dark matter, but they have been ...
Yue Shen   +10 more
doaj   +1 more source

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