Results 191 to 200 of about 97,087 (224)
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Surveying the distant Universe. [PDF]
van Kampen E +29 more
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Evidence for a sub-Jovian planet in the young TWA 7 disk. [PDF]
Lagrange AM +28 more
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A luminous and young galaxy at z = 12.33 revealed by a JWST/MIRI detection of Hα and [O iii]. [PDF]
Zavala JA +39 more
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A cosmic-ray loaded nascent outflow driven by a massive star cluster. [PDF]
Lemoine-Goumard M +8 more
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Star formation shut down by multiphase gas outflow in a galaxy at a redshift of 2.45. [PDF]
Belli S +17 more
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The most energetic transients: Tidal disruptions of high-mass stars. [PDF]
Hinkle JT +15 more
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Reading signatures of supermassive binary black holes in pulsar timing array observations. [PDF]
Goncharov B +12 more
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Distant radio galaxies and their environments [PDF]
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
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Radio Galaxies and Their Environment
2002In 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
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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
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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

