Results 191 to 200 of about 97,087 (224)

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Surveying the distant Universe. [PDF]

open access: yesOpen Res Eur
van Kampen E   +29 more
europepmc   +1 more source

Evidence for a sub-Jovian planet in the young TWA 7 disk. [PDF]

open access: yesNature
Lagrange AM   +28 more
europepmc   +1 more source

A luminous and young galaxy at z = 12.33 revealed by a JWST/MIRI detection of Hα and [O iii]. [PDF]

open access: yesNat Astron
Zavala JA   +39 more
europepmc   +1 more source

A cosmic-ray loaded nascent outflow driven by a massive star cluster. [PDF]

open access: yesNat Commun
Lemoine-Goumard M   +8 more
europepmc   +1 more source

Star formation shut down by multiphase gas outflow in a galaxy at a redshift of 2.45. [PDF]

open access: yesNature
Belli S   +17 more
europepmc   +1 more source

The most energetic transients: Tidal disruptions of high-mass stars. [PDF]

open access: yesSci Adv
Hinkle JT   +15 more
europepmc   +1 more source

Reading signatures of supermassive binary black holes in pulsar timing array observations. [PDF]

open access: yesNat Commun
Goncharov B   +12 more
europepmc   +1 more source

Distant radio galaxies and their environments [PDF]

open access: yesAstronomy and Astrophysics Review, 2008
82 pages, 20 figures. Accepted for publication in Astronomy and Astrophysics Reviews. Full resolution version available from http://www.springerlink.com/content/17123p4h8x6g0081/
C de Breuck
exaly   +3 more sources

Radio Galaxies and Their Environment

2002
In this paper we review the properties of radio galaxies in connection to the effect of the dynamic gaseous environment inside clusters in which they are embedded. The external gas can interact with a radio source in different ways: modifying its morphology via ram-pressure, confining the radio lobes, possibly feeding the active nucleus, enhancing star
Feretti L. 1, Venturi T. 1
openaire   +2 more sources

Radio Galaxies and Quasars

Annals of the New York Academy of Sciences, 1974
The discrete sources of radio emission were first distinguished from the general background radiation during the 1940’s as a result of their rapid amplitude scintillations ; and initially, it was thought that the scintillations were due to fluctuations in the intrinsic intensity of the discrete sources. Assuming that the dimensions of the sources could
openaire   +1 more source

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