227 research outputs found
Astrophysical Polarimetry of Cosmological Sources
Kostelecky and Mewes have recently shown that sensitive constraints can be
placed on some aspects of Lorentz symmetry violation using certain astronomical
data on high-redshift sources. Here, I introduce that data in its astronomical
context, making it clear that these data are robust and accurate for their
purpose. In particular, I explain that spatially extended scattered light from
obscured quasars leads to a centrosymmetric scattering polarization, with
polarization position angle independent of wavelength. Evidentally, these
relationships aren't spoiled by propagation effects as the photons cross the
universe.Comment: 7 pages, 4 figures, Second Meeting on CPT and Lorentz Symmetry,
Bloomington, IN (Aug. 2001
A First Close Look at the Balmer-edge Behavior of the Quasar Big Blue Bump
We have found for the first time a Balmer edge feature in the Big Blue Bump
emission of a quasar. The feature is seen in the polarized flux spectrum of the
quasar, where all the emissions from outside the nucleus are scraped off and
removed. The existence of the Balmer-edge absorption feature directly indicates
that the Big Blue Bump is indeed thermal and optically-thick.Comment: 2 pages, 2 figures. To be published in conference proceedings "Active
Galactic Nuclei: from Central Engine to Host Galaxy
Extremely Luminous Water Vapor Emission from a Type 2 Quasar at Redshift z = 0.66
A search for water masers in 47 Sloan Digital Sky Survey Type 2 quasars using
the Green Bank Telescope has yielded a detection at a redshift of z = 0.660.
This maser is more than an order of magnitude higher in redshift than any
previously known and, with a total isotropic luminosity of 23,000 L_sun, also
the most powerful. The presence and detectability of water masers in quasars at
z ~ 0.3-0.8 may provide a better understanding of quasar molecular tori and
disks, as well as fundamental quasar and galaxy properties such as black hole
masses. Water masers at cosmologically interesting distances may also
eventually provide, via direct distance determinations, a new cosmological
observable for testing the reality and properties of dark energy, currently
inferred primarily through Type 1a supernova measurements.Comment: 8 pages including 1 figure; accepted for publication in ApJ Letter
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