Results 1 to 10 of about 77,751 (271)
Spatially Resolved Spectra of 3C Galaxy Nuclei [PDF]
We present and discuss visible-wavelength long-slit spectra of four low redshift 3C galaxies obtained with the STIS instrument on the Hubble Space Telescope. The slit was aligned with near-nuclear jet-like structure seen in HST images of the galaxies, to give unprecedented spatial resolution of the galaxy inner regions.
J. B. Hutchings +5 more
core +7 more sources
The Role of AGN in Luminous Infrared Galaxies from the Multiwavelength Perspective
Galaxy mergers provide a mechanism for galaxies to effectively funnel gas and materials toward their nuclei and fuel the central starbursts and accretion of supermassive black holes.
Vivian U
doaj +1 more source
The origin of the low-ionization nuclear emission-line region (LINER) prevalent in local galaxies and its relationship with supermassive black holes have been debated for decades.
Zongnan Li +3 more
doaj +1 more source
Galaxies with Binary Nuclei [PDF]
AbstractIt is known that among active galaxies (AG) with strong emission lines (UV-galaxies, Sy1 and Sy2, Markarian and Kazarian galaxies, radio-galaxies, QSOs host galaxies and so on) there is a large percentage of objects with double and multiple (or complex) nuclei.
Yervant Terzian, Edward Khachikian
openaire +1 more source
SDSS-IV MaNGA: How Galaxy Interactions Influence Active Galactic Nuclei
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
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
Active galactic nuclei and galaxy interactions [PDF]
We perform a statistical analysis of active galactic nucleus (AGN) host characteristics and nuclear activity for AGNs in pairs and without companions. Our study concerns a sample of AGNs derived from the Sloan Digital Sky Survey Data Release 4 data by Kauffmann et al. and pair galaxies obtained from the same data set by Alonso et al.
Alonso, M. Sol +3 more
openaire +2 more sources
Eicheon properties are discussed. It is shown that the eicheon surface allows setting a boundary condition for the vacuum polarization and obtaining a solution describing the dark matter tail in the Milky Way Galaxy. That is, the dark matter in the Milky
Sergey L. Cherkas +1 more
doaj +1 more source
Dark Matter in the Milky Way as the F-Type of Vacuum Polarization
Dark matter in the Milky Way is explained by the F-type of vacuum polarization, which could represent dark radiation. A nonsingular solution for dark radiation exists in the presence of eicheon (i.e., black hole in old terminology) in the galaxy’s center.
Sergey L. Cherkas +1 more
doaj +1 more source
Young nuclei in dwarf elliptical galaxies [PDF]
accepted to "Astronomy Letters". Version for astro-ph with colour figures.
Chilingarian, Igor V. +3 more
openaire +2 more sources

