192 research outputs found
GALEX and Optical Light Curves of EF Eridanus During a Low State: the Puzzling Source of UV Light
Low state optical photometry of EF Eri during an extended low accretion state
combined with GALEX near and far UV time-resolved photometry reveals a source
of UV flux that is much larger than the underlying 9500K white dwarf, and that
is highly modulated on the orbital period. The near UV and optical light curves
can be modeled with a 20,000K spot but no spot model can explain both the large
amplitude FUV variations and the SED. The limitations of limb darkening,
cyclotron and magnetic white dwarf models in explaining the observations are
discussed.Comment: 10 pages, 4 figures to be published in ApJ Letter
X-ray and Multiwavelength Insights into the Nature of Weak Emission-Line Quasars at Low Redshift
(Abridged) We report on the X-ray and multiwavelength properties of 11
radio-quiet quasars with weak or no emission lines identified by the Sloan
Digital Sky Survey (SDSS) with redshift z=0.4-2.5. The distribution of relative
X-ray brightness for our low-redshift weak-line quasar (WLQ) candidates is
significantly different from that of typical radio-quiet quasars, having an
excess of X-ray weak sources, but it is consistent with that of high-redshift
WLQs. The X-ray weak sources generally show similar UV emission-line properties
to those of the X-ray weak quasar PHL 1811; they may belong to the notable
class of PHL 1811 analogs. The average X-ray spectrum of these sources is
somewhat harder than that of typical radio-quiet quasars. Several other
low-redshift WLQ candidates have normal ratios of X-ray-to-optical/UV flux, and
their average X-ray spectral properties are also similar to those of typical
radio-quiet quasars. The X-ray weak and X-ray normal WLQ candidates may belong
to the same subset of quasars having high-ionization "shielding gas" covering
most of the wind-dominated broad emission-line region, but be viewed at
different inclinations. The mid-infrared-to-X-ray spectral energy distributions
(SEDs) of these sources are generally consistent with those of typical SDSS
quasars, showing that they are not likely to be BL Lac objects with
relativistically boosted continua and diluted emission lines. However, one
source in our X-ray observed sample is remarkably strong in X-rays, indicating
that a small fraction of low-redshift WLQ candidates may actually be BL Lacs
residing in the radio-faint tail of the BL Lac population. We also investigate
universal selection criteria for WLQs over a wide range of redshift, finding
that it is not possible to select WLQ candidates in a fully consistent way
using different prominent emission lines as a function of redshift.Comment: ApJ in press; 26 pages, 11 figures and 7 tables. The full Table 3 is
available upon reques
The Ultraviolet-to-Mid-Infrared Spectral Energy Distribution of Weak Emission Line Quasars
We present Spitzer Space Telescope photometry of 18 Sloan Digital Sky Survey
(SDSS) quasars at 2.7 <= z <= 5.9 which have weak or undetectable
high-ionization emission lines in their rest-frame ultraviolet (UV) spectra
(hereafter weak-lined quasars, or WLQs). The Spitzer data are combined with
SDSS spectra and ground-based, near-infrared (IR) photometry of these sources
to produce a large inventory of spectral energy distributions (SEDs) of WLQs
across the rest-frame ~0.1-5 mum spectral band. The SEDs of our sources are
inconsistent with those of BL Lacertae objects which are dominated by
synchrotron emission due to a jet aligned close to our line-of-sight, but are
consistent with the SED of ordinary quasars with similar luminosities and
redshifts that exhibit a near-to-mid-IR 'bump', characteristic of hot dust
emission. This indicates that broad emission lines in WLQs are intrinsically
weak, rather than suffering continuum dilution from a jet, and that such
sources cannot be selected efficiently from traditional photometric surveys.Comment: 10 pages (emulateapj), 4 figures. Accepted for publication in Ap
Circular Polarization Variability in Extragalactic Sources on Time Scales of Months to Decades
We present previously unpublished circular polarization (cp) measurementsat 4.8 and 8.0 GHz made with the University of Michigan 26-meter primefocus telescope during 1978–1984 and results of a newobservational program during the past two years. Based on the preliminary analysis of our recent data, eight sources were detected at 4.8 GHz with average degrees of cp ranging from ≤ 0.1% to ≥ 1%.The results are compared with observations at other frequencies and with linearpolarization and total flux density variability in the sources.The behavior of the cp variability observed to date is consistentwith stochastic variations produced by mode conversion in transient,opaque emitting regions in the sources. The observed sign changes observedbetween different epochs and different frequencies are not consistentwith the hypothesis that sources maintain a fixed handedness of cp.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/42005/1/10509_2004_Article_5252793.pd
The X-ray Point Source Population Hosted by Globular Clusters in the Elliptical Galaxy NGC 4261
Utilising archival Chandra X-ray Observatory data and Hubble Space Telescope
globular cluster catalogues, we probe the time-domain properties of the low
mass X-ray binary population in the elliptical galaxy NGC 4261. Of the 98
unique X-ray sources identified in this study, 62 sources are within the
optical field of view and, of those, 33% are aligned with an optical cluster
counterpart. We find twenty X-ray sources coincident with globular clusters;
two are previously discovered ultra-luminous X-ray sources (ULXs) and eighteen
are low mass X-ray binaries (GCLMXBs) with erg s. ULXs
are a heterogeneous class of extremely bright X-ray binaries (
erg s) and ULXs located in globular clusters (GCULXs) and may be
indicators of black holes. Identifying these unusually X-ray bright sources and
measuring their optical properties can provide valuable constraints on the
progenitors of gravitational wave sources. We compare observations of these
sources to the twenty previously-studied GCULXs from five other early-type
galaxies, and find that GCULXs in NGC 4261 are of similar colour and luminosity
and do not significantly deviate from the rest of the sample in terms of
distance from the galaxy centre or X-ray luminosity. Both the GCULX and low
mass X-ray binary (GCLMXB) populations of NGC 4261 show long term variability;
the former may have implications for fast radio bursts originating in globular
clusters and the latter will likely introduce additional scatter into the low
mass end of GCLMXB X-ray luminosity functions.Comment: Accepted to MNRA
GALEX, Optical and IR Light Curves of MQ Dra: UV Excesses at Low Accretion Rates
Ultraviolet light curves constructed from NUV and FUV detectors on GALEX
reveal large amplitude variations during the orbital period of the Low
Accretion Rate Polar MQ Dra (SDSSJ1553+55). This unexpected variation from a UV
source is similar to that seen and discussed in the Polar EF Eri during its low
state of accretion, even though the accretion rate in MQ Dra is an order of
magnitude lower than even the low state of EF Eri. The similarity in phasing of
the UV and optical light curves in MQ Dra imply a similar location for the
source of light. We explore the possibilities of hot spots and cyclotron
emission with simple models fit to the UV, optical and IR light curves of MQ
Dra. To match the GALEX light curves with a single temperature circular hot
spot requires different sizes of spots for the NUV and FUV, while a cyclotron
model that can produce the optical harmonics with a magnetic field near 60 MG
requires multipoles with fields > 200 MG to match the UV fluxes.Comment: accepted for ApJ; 15 pages, 7 tables, 8 fig
The Relationship Between Fractures and DXA Measures of BMD in the Distal Femur of Children and Adolescents With Cerebral Palsy or Muscular Dystrophy
Children with limited or no ability to ambulate frequently sustain fragility fractures. Joint contractures, scoliosis, hip dysplasia, and metallic implants often prevent reliable measures of bone mineral density (BMD) in the proximal femur and lumbar spine, where BMD is commonly measured. Further, the relevance of lumbar spine BMD to fracture risk in this population is questionable. In an effort to obtain bone density measures that are both technically feasible and clinically relevant, a technique was developed involving dual-energy X-ray absorptiometry (DXA) measures of the distal femur projected in the lateral plane. The purpose of this study is to test the hypothesis that these new measures of BMD correlate with fractures in children with limited or no ability to ambulate. The relationship between distal femur BMD Z-scores and fracture history was assessed in a cross-sectional study of 619 children aged 6 to 18 years with muscular dystrophy or moderate to severe cerebral palsy compiled from eight centers. There was a strong correlation between fracture history and BMD Z-scores in the distal femur; 35% to 42% of those with BMD Z-scores less than −5 had fractured compared with 13% to 15% of those with BMD Z-scores greater than −1. Risk ratios were 1.06 to 1.15 (95% confidence interval 1.04–1.22), meaning a 6% to 15% increased risk of fracture with each 1.0 decrease in BMD Z-score. In clinical practice, DXA measure of BMD in the distal femur is the technique of choice for the assessment of children with impaired mobility. © 2010 American Society for Bone and Mineral Researc
Optically Selected BL Lacertae Candidates from the Sloan Digital Sky Survey Data Release Seven
We present a sample of 723 optically selected BL Lac candidates from the SDSS
DR7 spectroscopic database encompassing 8250 deg^2 of sky; our sample
constitutes one of the largest uniform BL Lac samples yet derived. Each BL Lac
candidate has a high-quality SDSS spectrum from which we determine
spectroscopic redshifts for ~60% of the objects. Redshift lower limits are
estimated for the remaining objects utilizing the lack of host galaxy flux
contamination in their optical spectra; we find that objects lacking
spectroscopic redshifts are likely at systematically higher redshifts.
Approximately 80% of our BL Lac candidates match to a radio source in
FIRST/NVSS, and ~40% match to a ROSAT X-ray source. The homogeneous
multiwavelength coverage allows subdivision of the sample into 637 radio-loud
BL Lac candidates and 86 weak-featured radio-quiet objects. The radio-loud
objects broadly support the standard paradigm unifying BL Lac objects with
beamed radio galaxies. We propose that the majority of the radio-quiet objects
may be lower-redshift (z<2.2) analogs to high-redshift weak line quasars (i.e.,
AGN with unusually anemic broad emission line regions). These would constitute
the largest sample of such objects, being of similar size and complementary in
redshift to the samples of high-redshift weak line quasars previously
discovered by the SDSS. However, some fraction of the weak-featured radio-quiet
objects may instead populate a rare and extreme radio-weak tail of the much
larger radio-loud BL Lac population. Serendipitous discoveries of unusual white
dwarfs, high-redshift weak line quasars, and broad absorption line quasars with
extreme continuum dropoffs blueward of rest-frame 2800 Angstroms are also
briefly described.Comment: 24 pages, 14 figures, 8 tables. Accepted for publication in A
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