0000000000587906

AUTHOR

J.m. Marcaide

showing 3 related works from this author

VLBI imaging of the gravitational lens MGJ0414+0534

2000

6 pages, 3 figures, accepted for publication in Astronomy & Astrophysics.-- Final full-text version of the paper available at: http://aa.springer.de/papers/0362003/2300845.pdf

GeneralLiterature_INTRODUCTORYANDSURVEYAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesquasars: individual: MGJ0414+0534 [Galaxies]Astrophysics::Cosmology and Extragalactic Astrophysicsgravitational lensing [Cosmology]AstrophysicsGalaxies: jetsTechniques: interferometricComputingMethodologies_DOCUMENTANDTEXTPROCESSINGGalaxies: quasars: individual: MGJ0414+0534interferometric [Techniques]jets [Galaxies]Cosmology: gravitational lensingAstrophysics::Galaxy Astrophysics
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Imaging of SN 1993J

2005

SN 1993J has been imaged with VLBI, and its angular expansion monitored, for almost ten years. The images show shell-like radio structures with almost circular symmetry. SN 1993J expands according to models of shock excited emission. The angular expansion has a changing deceleration rate and is best modeled with two different slopes. The swept-up mass estimate at an age of 3159 days (∼0.4 M⨀), comparable to the low-mass envelope, favors a binary scenario. The observed spectral index of SN 1993J has slowly flattened since age 1000 days onward (α has changed from −1 to −0.67 at an age of 2820 days).

PhysicsSpectral indexDeceleration parameterShock (fluid dynamics)Excited stateVery-long-baseline interferometryAstrophysicsCircular symmetryEnvelope (waves)
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New sample of large angular size radio galaxies. I.

2001

We present a new sample of 84 large angular size radio galaxies selected from the NRAO VLA Sky Survey. Radio sources with declination above +60{deg}, total flux density greater than 100mJy at 1.4GHz and angular size larger than 4' have been selected and observed with the VLA at 1.4 and 4.9GHz. The radio observations attempt to confirm the large angular size sources and to isolate the core emission for optical identification. In this paper, the first of a series of three, we present radio maps of 79 sources from the sample and discuss the effects of the selection criteria in the final sample. 37 radio galaxies belong to the class of giants, of which 22 are reported in this paper for the firs…

galactic and extragalactic astronomyAstrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaRadio galaxiesPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxiesNatural SciencesComputer Science::Digital LibrariesAstrophysics::Galaxy Astrophysics
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