29 research outputs found
On Quasar Masses and Quasar Host Galaxies
The mass of massive black holes in quasar cores can be deduced using the
typical velocities of Hb-emitting clouds in the Broad Line Region (BLR) and the
size of this region. However, this estimate depends on various assumptions and
is susceptible to large systematic errors. The Hb-deduced black hole mass in a
sample of 14 bright quasars is found here to correlate with the quasar host
galaxy luminosity, as determined with the Hubble Space Telescope (HST). This
correlation is similar to the black hole mass vs. bulge luminosity correlation
found by Magorrian et al. in a sample of 32 nearby normal galaxies. The
similarity of the two correlations is remarkable since the two samples involve
apparently different types of objects and since the black hole mass estimates
in quasars and in nearby galaxies are based on very different methods.
This similarity provides a ``calibration'' of the Hb-deduced black hole mass
estimate, suggesting it is accurate to +-0.5 on log scale. The similarity of
the two correlations also suggests that quasars reside in otherwise normal
galaxies, and that the luminosity of quasar hosts can be estimated to +-0.5 mag
based on the quasar continuum luminosity and the Hb line width. Future imaging
observations of additional broad-line active galaxies with the HST are required
in order to explore the extent, slope, and scatter of the black hole mass vs.
host bulge luminosity correlation in active galaxies.Comment: Accepted for publication in ApJ Letters, 7 pages, aas2pp4.st
AGN Black Hole Masses and Bolometric Luminosities
Black hole mass, along with mass accretion rate, is a fundamental property of
active galactic nuclei. Black hole mass sets an approximate upper limit to AGN
energetics via the Eddington limit. We collect and compare all AGN black hole
mass estimates from the literature; these 177 masses are mostly based on the
virial assumption for the broad emission lines, with the broad-line region size
determined from either reverberation mapping or optical luminosity. We
introduce 200 additional black hole mass estimates based on properties of the
host galaxy bulges, using either the observed stellar velocity dispersion or
using the fundamental plane relation to infer ; these methods assume
that AGN hosts are normal galaxies. We compare 36 cases for which black hole
mass has been generated by different methods and find, for individual objects,
a scatter as high as a couple of orders of magnitude. The less direct the
method, the larger the discrepancy with other estimates, probably due to the
large scatter in the underlying correlations assumed. Using published fluxes,
we calculate bolometric luminosities for 234 AGNs and investigate the relation
between black hole mass and luminosity. In contrast to other studies, we find
no significant correlation of black hole mass with luminosity, other than those
induced by circular reasoning in the estimation of black hole mass. The
Eddington limit defines an approximate upper envelope to the distribution of
luminosities, but the lower envelope depends entirely on the sample of AGN
included. For any given black hole mass, there is a range in Eddington ratio of
up to three orders of magnitude.Comment: 43 pages with 10 figures. Accepted for publication in Ap
Dynamical Mass of Type 2 Seyfert Nuclei
We have derived the masses of central objects () of nine type 2
Seyfert nuclei using the observational properties of the hidden broad H
emission. We obtain the average dynamical mass, log where is the optical depth
for electron scattering. If , this average mass is almost
comparable with those of type 1 Seyfert nuclei. However, if ,
as is usually considered, the average mass of type 2 Seyfert nuclei may be more
massive than that of type 1s. We discuss implications for issues concerning
both the current unified model of Seyfert nuclei and physical conditions of the
electron scattering regions.Comment: 21 pages, 2 figures; accepted for Astrophysical Journa
Evidence for the evolutionary sequence of blazars: different types of accretion flows in BL Lac objects
The limits on the mass of the black hole in 23 BL Lac objects are obtained
from their luminosities of the broad emission line H\beta on the assumption
that broad emission lines are emitted from clouds ionized by the radiation of
the accretion disk surrounding a black hole. The distribution of line
luminosity L_{H\beta} of all these BL Lac objects suggests a bimodal nature,
although this cannot be statistically proven on the basis of the present,
rather small sample. We found that standard thin disks are probably in the
sources with L_{H\beta}>10^{41} erg s^{-1}. The central black holes in these
sources have masses of 10^{8-10} M_\odot, if the matter is accreting at the
rate of 0.025 {\dot M}_{\rm Edd}. For the sources with L_{H\beta}<10^{41} erg
s^{-1}, the accretion flows have transited from standard thin disk type to the
ADAF type. The lower limits on the mass of the black hole in these sources are
in the range of 1.66-24.5\times 10^{8} M_\odot. The results support the
evolutionary sequence of blazars: FSRQ\to LBL\to HBL.Comment: 5 pages, accepted for publication in ApJ Letter
Correlação entre Capacidade Funcional e Qualidade de Vida em Pacientes Oncológicos em Cuidados Paliativos
Introdução: Cuidados paliativos sĂŁo descritos como um conjunto de terapĂȘuticas que visam minimizar as implicaçÔes negativas das doenças graves que ameaçam a vida e o bem-estar do indivĂduo acometido. A progressĂŁo da doença e a sintomatologia provocam uma deterioração gradual e generalizada do estado do doente, e os sintomas fĂsicos ocasionam a perda progressiva da capacidade funcional que, associados Ă s manifestaçÔes emocionais pelo momento em que o paciente se encontra, impactam a sua qualidade de vida. Objetivo: Correlacionar a capacidade funcional com a qualidade de vida de pacientes oncolĂłgicos em cuidados paliativos. MĂ©todo: Estudo transversal de abordagem quantitativa com 225 indivĂduos. Os dados foram coletados por meio de questionĂĄrio sociodemogrĂĄfico, do Ăndice de Barthel e do European Organization for Research in the Treatment of Cancer Questionnaire Palliative (EORTC QLQ-C15-PAL). Resultados: Dos 225 indivĂduos elegĂveis, observou-se homogeneidade entre a porcentagem de homens e mulheres, com mĂ©dia de 55,73±15,14 anos de idade. A anĂĄlise estatĂstica demonstrou associação positiva entre o escore do Ăndice de Barthel e o escore de qualidade de vida do EORTC QLQ-C15-PAL com coeficiente de 0,74 e nĂvel significĂąncia de p<0,05, bem como correlação negativa para as subescalas funcional e de sintomas com coeficiente de -0,702 e -0,544, respectivamente. ConclusĂŁo: HĂĄ uma correlação significativa entre a capacidade funcional e a qualidade de vida em pacientes oncolĂłgicos em cuidados paliativos
The Updated Zwicky Catalog (UZC)
The Zwicky Catalog of galaxies (ZC), with m_Zw<=15.5mag, has been the basis
for the Center for Astrophysics (CfA) redshift surveys. To date, analyses of
the ZC and redshift surveys based on it have relied on heterogeneous sets of
galaxy coordinates and redshifts. Here we correct some of the inadequacies of
previous catalogs by providing: (1) coordinates with <~2 arcsec errors for all
of the Nuzc catalog galaxies, (2) homogeneously estimated redshifts for the
majority (98%) of the data taken at the CfA (14,632 spectra), and (3) an
estimate of the remaining "blunder" rate for both the CfA redshifts and for
those compiled from the literature. For the reanalyzed CfA data we include a
calibrated, uniformly determined error and an indication of the presence of
emission lines in each spectrum. We provide redshifts for 7,257 galaxies in the
CfA2 redshift survey not previously published; for another 5,625 CfA redshifts
we list the remeasured or uniformly re-reduced value. Among our new
measurements, Nmul are members of UZC "multiplets" associated with the original
Zwicky catalog position in the coordinate range where the catalog is 98%
complete. These multiplets provide new candidates for examination of tidal
interactions among galaxies. All of the new redshifts correspond to UZC
galaxies with properties recorded in the CfA redshift compilation known as
ZCAT. About 1,000 of our new measurements were motivated either by inadequate
signal-to-noise in the original spectrum or by an ambiguous identification of
the galaxy associated with a ZCAT redshift. The redshift catalog we include
here is ~96% complete to m_Zw<=15.5, and ~98% complete (12,925 galaxies out of
a total of 13,150) for the RA(1950) ranges [20h--4h] and [8h--17h] and
DEC(1950) range [-2.5d--50d]. (abridged)Comment: 34 pp, 7 figs, PASP 1999, 111, 43
The accuracy of supermassive black hole masses determined by the single-epoch spectrum (Dibai) method
A possible relation between the masses of black holes in galactic nuclei and the parameters of the host galaxies
Reliability of different methodologies of infrared image analysis of myofascial trigger points in the upper trapezius muscle
BACKGROUND: Infrared thermography is recognized as a viable method for evaluation of subjects with myofascial pain. OBJECTIVE: The aim of the present study was to assess the intra- and inter-rater reliability of infrared image analysis of myofascial trigger points in the upper trapezius muscle. METHOD: A reliability study was conducted with 24 volunteers of both genders (23 females) between 18 and 30 years of age (22.12±2.54), all having cervical pain and presence of active myofascial trigger point in the upper trapezius muscle. Two trained examiners performed analysis of point, line, and area of the infrared images at two different periods with a 1-week interval. The intra-class correlation coefficient (ICC2,1) was used to assess the intra- and inter-rater reliability. RESULTS: With regard to the intra-rater reliability, ICC values were between 0.591 and 0.993, with temperatures between 0.13 and 1.57 °C for values of standard error of measurement (SEM) and between 0.36 and 4.35 °C for the minimal detectable change (MDC). For the inter-rater reliability, ICC ranged from 0.615 to 0.918, with temperatures between 0.43 and 1.22 °C for the SEM and between 1.19 and 3.38 °C for the MDC. CONCLUSION: The methods of infrared image analyses of myofascial trigger points in the upper trapezius muscle employed in the present study are suitable for clinical and research practices