Asset Details
MbrlCatalogueTitleDetail
Do you wish to reserve the book?
An Elusive Population of Massive Disk Galaxies Hosting Double-lobed Radio-loud Active Galactic Nuclei
by
Ho, Luis C
, Zhuang, Ming-Yang
, Wu, Zihao
in
Active galactic nuclei
/ Alignment
/ Black holes
/ Cosmic dust
/ Disk galaxies
/ Elliptical galaxies
/ Galactic bulge
/ Galactic structure
/ Galaxies
/ Hubble Space Telescope
/ Lobes
/ Morphology
/ Optical counterparts (astronomy)
/ Radio galaxies
/ Radio jets (astronomy)
/ Space telescopes
/ Stellar mass
2022
Hey, we have placed the reservation for you!
By the way, why not check out events that you can attend while you pick your title.
You are currently in the queue to collect this book. You will be notified once it is your turn to collect the book.
Oops! Something went wrong.
Looks like we were not able to place the reservation. Kindly try again later.
Are you sure you want to remove the book from the shelf?
An Elusive Population of Massive Disk Galaxies Hosting Double-lobed Radio-loud Active Galactic Nuclei
by
Ho, Luis C
, Zhuang, Ming-Yang
, Wu, Zihao
in
Active galactic nuclei
/ Alignment
/ Black holes
/ Cosmic dust
/ Disk galaxies
/ Elliptical galaxies
/ Galactic bulge
/ Galactic structure
/ Galaxies
/ Hubble Space Telescope
/ Lobes
/ Morphology
/ Optical counterparts (astronomy)
/ Radio galaxies
/ Radio jets (astronomy)
/ Space telescopes
/ Stellar mass
2022
Oops! Something went wrong.
While trying to remove the title from your shelf something went wrong :( Kindly try again later!
Do you wish to request the book?
An Elusive Population of Massive Disk Galaxies Hosting Double-lobed Radio-loud Active Galactic Nuclei
by
Ho, Luis C
, Zhuang, Ming-Yang
, Wu, Zihao
in
Active galactic nuclei
/ Alignment
/ Black holes
/ Cosmic dust
/ Disk galaxies
/ Elliptical galaxies
/ Galactic bulge
/ Galactic structure
/ Galaxies
/ Hubble Space Telescope
/ Lobes
/ Morphology
/ Optical counterparts (astronomy)
/ Radio galaxies
/ Radio jets (astronomy)
/ Space telescopes
/ Stellar mass
2022
Please be aware that the book you have requested cannot be checked out. If you would like to checkout this book, you can reserve another copy
We have requested the book for you!
Your request is successful and it will be processed during the Library working hours. Please check the status of your request in My Requests.
Oops! Something went wrong.
Looks like we were not able to place your request. Kindly try again later.
An Elusive Population of Massive Disk Galaxies Hosting Double-lobed Radio-loud Active Galactic Nuclei
Journal Article
An Elusive Population of Massive Disk Galaxies Hosting Double-lobed Radio-loud Active Galactic Nuclei
2022
Request Book From Autostore
and Choose the Collection Method
Overview
It is commonly accepted that radio-loud active galactic nuclei are hosted exclusively by giant elliptical galaxies. We analyze high-resolution optical Hubble Space Telescope images of a sample of radio galaxies with extended double-lobed structures associated with disk-like optical counterparts. After systematically evaluating the probability of chance alignment between the radio lobes and the optical counterparts, we obtain a sample of 18 objects likely to have genuine associations. The host galaxies have unambiguous late-type morphologies, including spiral arms, large-scale dust lanes among the edge-on systems, and exceptionally weak bulges, as judged by the low global concentrations, small global Sérsic indices, and low bulge-to-total light ratios (median B/T = 0.13). With a median Sérsic index of 1.4 and low effective surface brightnesses, the bulges are consistent with being pseudobulges. The majority of the hosts have unusually large stellar masses (median M * = 1.3 × 1011 M ⊙) and red optical colors (median g − r = 0.69 mag), consistent with massive, quiescent galaxies on the red sequence. We suggest that the black hole mass (stellar mass) plays a fundamental role in launching large-scale radio jets, and that the rarity of extended radio lobes in late-type galaxies is the consequence of the steep stellar mass function at the high-mass end. The disk radio galaxies have mostly Fanaroff–Riley type II morphologies yet lower radio power than sources of a similar type traditionally hosted by ellipticals. The radio jets show no preferential alignment with the minor axis of the galactic bulge or disk, apart from a possible mild tendency for alignment among the most disk-dominated systems.
Publisher
IOP Publishing
Subject
This website uses cookies to ensure you get the best experience on our website.