129 research outputs found
X-ray sources in globular clusters
Observations with BeppoSAX, RXTE and Chandra suggest that many of the bright
X-ray sources in globular clusters have ultrashort binary periods. This is
remarkable as such systems are not easily formed. With accurate optical
astrometry of HST images, the large numbers of low-luminosity X-ray sources
discovered with Chandra can be classified as quiescent low-mass X-ray binaries,
pulsars, cataclysmic variables, and magnetically active binaries. The number of
cataclysmic variables is found to scale with the number of close stellar
encounters.Comment: Invited review in: "Interacting binaries", July 4-10 Cefalu, eds.
Antonelli et al., to be published with AIP. 10 pages,6 figure
A new look at distances and velocities of neutron stars
We take a fresh look at the determination of distances and velocities of
neutron stars. The conversion of a parallax measurement into a distance, or
distance probability distribution, has led to a debate quite similar to the one
involving Cepheids, centering on the question whether priors can be used when
discussing a single system. With the example of PSRJ0218+4232 we show that a
prior is necessary to determine the probability distribution for the distance.
The distance of this pulsar implies a gamma-ray luminosity larger than 10% of
its spindown luminosity. For velocities the debate is whether a single
Maxwellian describes the distribution for young pulsars. By limiting our
discussion to accurate (VLBI) measurements we argue that a description with two
Maxwellians, with distribution parameters sigma1=77 and sigma2=320 km/s, is
significantly better. Corrections for galactic rotation, to derive velocities
with respect to the local standards of rest, are insignificant.Comment: Has appeared in Journal of Astrophysics and Astronomy special issue
on 'Physics of Neutron Stars and Related Objects', celebrating the 75th
birth-year of G. Srinivasan. Ten pages, nine figure
Observational evidence for the origin of X-ray sources in globular clusters
Low-mass X-ray binaries, recycled pulsars, cataclysmic variables and
magnetically active binaries are observed as X-ray sources in globular
clusters. We discuss the classification of these systems, and find that some
presumed active binaries are brighter than expected. We discuss a new
statistical method to determine from observations how the formation of X-ray
sources depends on the number of stellar encounters and/or on the cluster mass.
We show that cluster mass is not a proxy for the encounter number, and that
optical identifications are essential in proving the presence of primordial
binaries among the low-luminosity X-ray sources.Comment: 10 pages, 7 figures, to appear in IAUS 246, Dynamical evolution of
dense stellar systems, ed. E. Vesperin
The observed velocity distribution of young pulsars
We argue that comparison with observations of theoretical models for the
velocity distribution of pulsars must be done directly with the observed
quantities, i.e. parallax and the two components of proper motion. We develop a
formalism to do so, and apply it to pulsars with accurate VLBI measurements. We
find that a distribution with two maxwellians improves significantly on a
single maxwellian. The `mixed' model takes into account that pulsars move away
from their place of birth, a narrow region around the galactic plane. The best
model has 42% of the pulsars in a maxwellian with average velocity sigma
sqrt{8/pi}=120 km/s, and 58% in a maxwellian with average velocity 540 km/s.
About 5% of the pulsars has a velocity at birth less than 60\,km/s. For the
youngest pulsars (tau_c<10 Myr), these numbers are 32% with 130 km/s, 68% with
520 km/s, and 3%, with appreciable uncertainties.Comment: submitted to A&A; 14 pages, 10 figure
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