Results 81 to 90 of about 1,073,559 (305)

Radio and optical orientations of galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2009
We investigate the correlations between optical and radio isophotal position angles for 14302 SDSS galaxies with $r$ magnitudes brighter than 18 and which have been associated with extended FIRST radio sources. We identify two separate populations of galaxies using the colour, concentration and their principal components.
Battye, R. A., Browne, I. W A
openaire   +4 more sources

Optical and Radio Properties of Extragalactic Sources Observed by the FIRST and SDSS Surveys

open access: yes, 2002
We discuss the optical and radio properties of 30,000 FIRST sources positionally associated with an SDSS source in 1230 deg$^2$ of sky. The majority (83%) of the FIRST sources identified with an SDSS source brighter than r=21 are optically resolved.
Ali Kinkhabwala   +46 more
core   +1 more source

Discovery of rare double-lobe radio galaxies hosted in spiral galaxies [PDF]

open access: yes, 2015
Double-lobe radio galaxies in the local Universe have traditionally been found to be hosted in elliptical or lenticular galaxies. We report the discovery of four spiral-host double-lobe radio galaxies (J0836+0532, J1159+5820, J1352+3126 and J1649+2635 ...
Veeresh Singh   +5 more
semanticscholar   +1 more source

CO Survey of High-z Radio Galaxies, Revisited with the Atacama Large Millimeter/submillimeter Array: Jet–Cloud Alignments and Synchrotron Brightening by Molecular Gas in the Circumgalactic Environment

open access: yesThe Astrophysical Journal, 2023
Powerful radio sources associated with supermassive black holes are among the most luminous objects in the universe, and are frequently recognized both as cosmological probes and active constituents in the evolution of galaxies.
Bjorn H. C. Emonts   +8 more
doaj   +1 more source

The Environments of Low and High Luminosity Radio Galaxies at Moderate Redshifts

open access: yes, 2008
In the local Universe, high-power radio galaxies live in lower density environments than low-luminosity radio galaxies. If this trend continues to higher redshifts, powerful radio galaxies would serve as efficient probes of moderate redshift groups and ...
Aceves   +20 more
core   +1 more source

Associating Fast Radio Bursts with Their Host Galaxies [PDF]

open access: yes, 2017
The first precise localization of a fast radio burst (FRB) sheds light on the nature of these mysterious bursts and the physical mechanisms that power them.
T. Eftekhari, E. Berger
semanticscholar   +1 more source

Dust tori in radio galaxies [PDF]

open access: yesAstronomy and Astrophysics, 2010
17 pages, 9 figures, published in Astronomy and Astrophysics. Version 2 matches published version.
J. W. Pel   +3 more
openaire   +5 more sources

Compliant Robotics in Space: A Prospective Review of Soft and Deformable Systems for Space Missions

open access: yesAdvanced Intelligent Systems, EarlyView.
Compliant robots are increasingly becoming integral to space exploration due to their adaptability, flexibility, and lightweight design. This article reviews categories such as soft, reconfigurable, and hyper‐redundant robots and their evolving role in enhancing space missions.
Hamed Rahimi Nohooji, Holger Voos
wiley   +1 more source

CHANG-ES IX: Radio scale heights and scale lengths of a consistent sample of 13 spiral galaxies seen edge-on and their correlations [PDF]

open access: yes, 2017
The vertical halo scale height is a crucial parameter to understand the transport of cosmic-ray electrons (CRE) and their energy loss mechanisms in spiral galaxies.
M. Krause   +16 more
semanticscholar   +1 more source

HI absorption in Radio Galaxies [PDF]

open access: yesSymposium - International Astronomical Union, 2002
Twenty-two powerful radio galaxies have been searched for HI absorption. We find the highest probability of detecting HI in absorption among narrow-line compact (or small) galaxies or galaxies with indication of richer interstellar medium (i.e. with ongoing or recent star-formation).
Tom Oosterloo   +4 more
openaire   +3 more sources

Home - About - Disclaimer - Privacy