Results 81 to 90 of about 881,876 (240)

Prospects for Observing Galaxy Spectral Energy Distribution from the Radio to the Far-infrared in the Era of Next-generation Radio Telescopes

open access: yesThe Astrophysical Journal
The superb sensitivity and angular resolution of the next-generation radio telescopes with combined frequency coverage of approximately over 3 orders of magnitude (100 MHz–100 GHz) will sample the radio and far-infrared (FIR) spectral energy distribution
Ilsang Yoon   +7 more
doaj   +1 more source

An HI+radio continuum study of local cluster galaxies

open access: yesAstronomy & Astrophysics
The evolution of galaxies in clusters is driven by their interaction with the environment. This deeply affects and alters the properties of the multiphase interstellar medium.
Ignesti Alessandro   +16 more
doaj   +1 more source

Pair-Matching of Radio-Loud and Radio-Quiet AGNs

open access: yesFrontiers in Astronomy and Space Sciences, 2017
Active galactic nuclei (AGNs) are known to cover an extremely broad range of radio luminosities and the spread of their radio-loudness is very large at any value of the Eddington ratio.
Dorota Kozieł-Wierzbowska   +5 more
doaj   +1 more source

Profiles of Anxiety in Children Undergoing Elective Surgery: Predictors and Perioperative Outcomes

open access: yesDevelopmental Psychobiology, Volume 68, Issue 5, September 2026.
ABSTRACT Surgery is an anxiety‐provoking event, but there are individual differences in the magnitude of experienced anxiety. The objective of this study was to identify patterns of children's preoperative anxiety, its predictors, and perioperative outcomes. The sample included 171 children (Mage = 9.95 years) undergoing elective surgery.
Kristie L. Poole   +5 more
wiley   +1 more source

On dynamical models for radio galaxies [PDF]

open access: yesNew Astronomy Reviews, 2002
The tailed radio galaxies that have been called ``Type I'' are not a uniform set. To study their dynamics, we have used the Ledlow-Owen data set, which provides a new sample of 250 radio galaxies in nearby Abell clusters. These sources divide into two clear categories based on their radio morphology.
Eilek, J.   +4 more
openaire   +2 more sources

Origin and Evolution of Large-scale Magnetic Fields [PDF]

open access: yes, 2015
Magnetic elds are ubiquitous at all scales in the Universe and have been observed in galaxies and clusters of galaxies via observations of di use radio emission and Faraday Rotation Measures.
Barnes, DJ
core  

Origin of the Double-peaked Narrow Emission Lines in the Optical Spectra of X-shaped Radio Galaxies

open access: yesThe Astrophysical Journal
We investigate X-shaped radio galaxies (XRGs) with optical double-peaked narrow emission lines (DPNELs) as potential hosts of dual or binary supermassive black holes (SMBHs).
Ghosh Prajnadipt   +15 more
doaj   +1 more source

MUC1 as a Survival Effector of Radiotherapy‐Induced Epithelial Hybrid States in Basal‐Like Breast Cancer

open access: yesInternational Journal of Cancer, Volume 159, Issue 5, Page 1296-1310, 1 September 2026.
Basal‐like breast cancer (BLBC) is aggressive and often exhibits inherent or acquired resistance to radiotherapy (RT), a primary treatment option. RT resistance is underpinned by molecular alterations, many of which are poorly understood. Here, RT‐induced transcriptomic changes were analyzed using bulk and spatial sequencing in a BLBC mouse model and ...
Garyfallia Pantelaiou‐Prokaki   +12 more
wiley   +1 more source

Testing the Correlation between Bending Angle and Polarization Properties of Bent Radio Galaxies

open access: yesThe Astrophysical Journal
The bending of radio galaxies in galaxy clusters is expected to be caused by interactions with the local environment. The physical processes responsible for jet bending, and their influence on the polarization properties of radio galaxies, remain poorly ...
S. Vanderwoude   +4 more
doaj   +1 more source

Large-Scale Environment Properties of Narrow-Line Seyfert 1 Galaxies at z < 0.4

open access: yesFrontiers in Astronomy and Space Sciences, 2017
The large-scale environment is believed to affect the evolution and intrinsic properties of galaxies. It offers a new perspective on narrow-line Seyfert 1 galaxies (NLS1) which have not been extensively studied in this context before.
Emilia Järvelä   +5 more
doaj   +1 more source

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