Quasar hosts. A workshop jointly organized by ESO and IAC, Puerto de la Cruz, Tenerife, 24 - 27 Sep 1996.
Not Available
Crane, P. et al.
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12
1996
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Quenching cluster cooling flows with recurrent hot plasma bubblesThe observed cooling rate of hot gas in clusters is much lower than that inferred from the gas density profiles. This suggests that the gas is being heated by some source. We use an adaptive-mesh refinement code (FLASH) to simulate the effect of multiple, randomly positioned, injections of thermal energy within 50 kpc of the centre of an initiallyDalla Vecchia, C. et al.
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122004 -
QUEST1 Variability Survey. II. Variability Determination Criteria and 200k Light Curve CatalogThe QUEST (QUasar Equatorial Survey Team) Phase 1 camera has collected multibandpass photometry on a large strip of high Galactic latitude sky over a period of 26 months. This robust data set has been reduced and nightly catalogs compared to determine the photometric variability of the ensemble objects. Subsequent spectroscopic observations haveRengstorf, A. W. et al.
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122004 -
Quiescent X-ray/optical counterparts of the black hole transient H 1705-250We report the result of a new Chandra observation of the black hole X-ray transient H 1705-250 in quiescence. H 1705-250 was barely detected in the new ˜50 ks Chandra observation. With five detected counts, we estimate the source quiescent luminosity to be LX ˜ 9.1 × 1030 erg s-1 in the 0.5-10 keV band (adopting a distance of 8.6 kpc). This valueWijnands, R. et al.
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122012 -
Quiet Solar Photosphere: Comparisons of High Resolution Observations with 3-D SimulationsNot AvailableCauzzi, G. et al.
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122005 -
Quiet-Sun Magnetic Fields: Simultaneous Inversion of Visible and IR Spectro-Polarimetric ObservationsWe studied the quiet-Sun magnetic fields interpreting spectro-polarimetric observations of infrared and visible spectral lines. Magnetic field strengths and filling factors were inferred by the simultaneous inversion of Stokes profiles of the Fe I lines at 6301.5, 6302.5, 15648, and 15653 Å under the MISMA hypothesis. They cover a solar intraDomínguez Cerdeña, I. et al.
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122006