84 research outputs found
An automated search for compact high-velocity clouds in the Leiden/Dwingeloo Survey
Wetensch. publicatieFaculteit der Wiskunde en Natuurwetenschappe
Onzekerheid over de baten van de Betuwelijn
Model estimates of the pay-off of the Betuwe railway have played an important role for politicians to decide to build this railway. This has already been discussed extensively, especially with respect to the macro-economic effects of this investment. A deeper analysis shows that these effects are very difficult to assess. The NIJFER institute for example calculated a long term profit of 52.1 biljon Dutch guilders, but our analysis of this model shows that the profitlays with 50 reliability between 15 and 30 biljon Dutch guilders. Our conclusion is that this political investment decision is not sufficiently supported by the expected macro-economic pay-off. A prudent use of quantitative research requires that the involved uncertainties in the model outcomes is properly taken into account.investment;cross-country analysis;regression;infrastructure;policy design
Onzekerheid over de baten van de Betuwelijn
Model estimates of the pay-off of the Betuwe railway have played an important role for politicians to decide to build this railway. This has already been discussed extensively, especially with respect to the macro-economic effects of this investment. A deeper analysis shows that these effects are very difficult to assess. The NIJFER institute for example calculated a long term profit of 52.1 biljon Dutch guilders, but our analysis of this model shows that the profit
lays with 50 reliability between 15 and 30 biljon Dutch guilders. Our conclusion is that this political investment decision is not sufficiently supported by the expected macro-economic pay-off. A prudent use of quantitative research requires that the involved uncertainties in the model outcomes is properly taken into account
Do the Unidentified EGRET Sources Trace Annihilating Dark Matter in the Local Group?
In a cold dark matter (CDM) framework of structure formation, the dark matter
haloes around galaxies assemble through successive mergers with smaller haloes.
This merging process is not completely efficient, and hundreds of surviving
halo cores, or {\it subhaloes}, are expected to remain in orbit within the halo
of a galaxy like the Milky Way. While the dozen visible satellites of the Milky
Way may trace some of these subhaloes, the majority are currently undetected. A
large number of high-velocity clouds (HVCs) of neutral hydrogen {\it are}
observed around the Milky Way, and it is plausible that some of the HVCs may
trace subhaloes undetected in the optical. Confirming the existence of
concentrations of dark matter associated with even a few of the HVCs would
represent a dramatic step forward in our attempts to understand the nature of
dark matter. Supersymmetric (SUSY) extensions of the Standard Model of particle
physics currently suggest neutralinos as a natural well-motivated candidate for
the non-baryonic dark matter of the universe. If this is indeed the case, then
it may be possible to detect dark matter indirectly as it annihilates into
neutrinos, photons or positrons. In particular, the centres of subhaloes might
show up as point sources in gamma-ray observations. In this work we consider
the possibility that some of the unidentified EGRET -ray sources trace
annihilating neutralino dark matter in the dark substructure of the Local
Group. We compare the observed positions and fluxes of both the unidentified
EGRET sources and the HVCs with the positions and fluxes predicted by a model
of halo substructure, to determine to what extent any of these three
populations could be associated.Comment: 12 Pages, 4 figures, to appear in a special issue of ApSS. Presented
at "The Multiwavelength Approach to Unidentified Gamma-Ray Sources" (Hong
Kong, June 1 - 4, 2004; Conference organizers: K.S. Cheng and G.E. Romero
High-resolution imaging of compact high-velocity clouds (II)
We have imaged five compact high-velocity clouds in HI with arcmin angular-
and km/s spectral-resolution using the WSRT. Supplementary total-power data,
which is fully sensitive to both the cool and warm components of HI, is
available for comparison for all the sources, albeit with angular resolutions
that vary from 3' to 36'. The fractional HI flux in compact CNM components
varies from 4% to 16% in our sample. All objects have at least one local peak
in the CNM column which exceeds about 10^19 cm^-2 when observed with arcmin
resolution. It is plausible that a peak column density of 1-2x10^19 cm^-2 is a
prerequisite for the long-term survival of these sources. One object in our
sample, CHVC120-20-443 (Davies' cloud), lies in close projected proximity to
the disk of M31. This object is characterized by exceptionally broad linewidths
in its CNM concentrations (more than 5 times greater than the median value).
These CNM concentrations lie in an arc on the edge of the source facing the M31
disk, while the diffuse HI component of this source has a position offset in
the direction of the disk. All of these attributes suggest that CHVC120-20-443
is in a different evolutionary state than most of the other CHVCs which have
been studied. Similarly broad CNM linewidths have only been detected in one
other object, CHVC111-07-466, which also lies in the Local Group barycenter
direction and has the most extreme radial velocity known. A distinct
possibility for Davies' cloud seems to be physical interaction of some type
with M31. The most likely form of this interaction might be the ram-pressure or
tidal- stripping by either one of M31's visible dwarf companions, M32 or
NGC205, or else by a dark companion with an associated HI condensation.Comment: 12 pages, 11 (low res.) png figs, accepted for pub. in A&
HIPASS High-Velocity Clouds: Properties of the Compact and Extended Populations
A catalog of Southern anomalous-velocity HI clouds at Decl. < +2 deg is
presented, based on data from the HI Parkes All-Sky Survey (HIPASS). The
improved sensitivity (5sigma: T_B = 0.04 K) and resolution (15.5') of the
HIPASS data results in a substantial increase in the number of individual
clouds (1956, as well as 41 galaxies) compared to previous surveys. Most
high-velocity emission features, HVCs, have a filamentary morphology and are
loosely organized into large complexes extending over tens of degrees. In
addition, 179 compact and isolated anomalous-velocity objects, CHVCs, are
identified based on their size and degree of isolation. 25% of the CHVCs
originally classified by Braun & Burton (1999) are reclassified. Both the
entire population of high-velocity emission features and the CHVCs alone have
typical HI masses of ~ 4.5 D(kpc)^2 solar masses and have similar slopes for
their column density and flux distributions. On the other hand, the CHVCs
appear to be clustered and the population can be broken up into three spatially
distinct groups, while the entire population of clouds is more uniformly
distributed with a significant percentage aligned with the Magellanic Stream.
The median velocities are V_GSR = -38 km/s for the CHVCs and -30 km/s for all
of the anomalous-velocity clouds. Based on the catalog sizes, high-velocity
features cover 19% of the southern sky and CHVCs cover 1%. (abridged)Comment: 32 pages, 26 figures in gif format, 2 ascii tables, to appear in the
Jan 2002 issue of The Astronomical Journal, high resolution version available
at http://origins.Colorado.EDU/~mputman/pubs.htm
Shot noise in ferromagnetic single electron tunneling devices
Frequency dependent current noise in ferromagnetic double junctions with
Coulomb blockade is studied theoretically in the limit of sequential tunneling.
Two different relaxation processes are found in the correlations between spin
polarized tunneling currents; low frequency spin fluctuations and high
frequency charge fluctuations. Spin accumulation in strongly asymmetric
junctions is shown to lead to a negative differential resistance. We also show
that large spin noise activated in the range of negative differential
resistance gives rise to a significant enhancement of the current noise.Comment: 8 pages, 13 eps-figures include
HI in Local Group analogs: what does it tell us about galaxy formation?
We present the results of our HI survey of six loose groups of galaxies
analogous to the Local Group. The survey was conducted using the Parkes
telescope and the Australia Telescope Compact Array to produce a census of all
the gas-rich galaxies and potential analogs to the high-velocity clouds (HVCs)
within these groups down to M(HI)<10^7 M(sun) as a test of models of galaxy
formation. We present the HI mass function and halo mass function for these
analogous groups and compare them with the Local Group and other environments.
We also demonstrate that our non-detection of HVC analogs in these groups
implies that they must have low HI masses and be clustered tightly around
galaxies, including around our own Milky Way, and are not distributed
throughout the Local Group.Comment: 5 pages, To appear in ESO Astrophysics Symposia: "Groups of Galaxies
in the Nearby Universe
An automated search for high-velocity clouds in the Leiden/Dwingeloo Survey
We describe an automated search through the Leiden/Dwingeloo HI Survey (LDS)
for high-velocity clouds north of Dec=-28 deg. From the general catalog we
extract a sample of isolated high-velocity clouds, CHVCs: anomalous-velocity HI
clouds which are sharply bounded in angular extent with no kinematic or spatial
connection to other HI features down to a limiting column density of
1.5*10^18cm^-2. This column density is an order of magnitude lower than the
critical HI column density, about 2*10^19cm^-2, where the ionized fraction is
thought to increase dramatically due to the extragalactic radiation field. As
such, these objects are likely to provide their own shielding to ionizing
radiation. Their small median angular size, of about 1 deg. FWHM, might then
imply substantial distances, since the partially ionized HI skin in a power-law
ionizing photon field has a typical exponential scale-length of 1 kpc. The
automated search algorithm has been applied to the HIPASS and to the
Leiden/Dwingeloo data sets. The results from the LDS are described here; Putman
et al. (2002) describe application of this algorithm to the HIPASS material. We
identify 67 CHVCs in the LDS which satisfy stringent requirements on isolation,
and an additional 49 objects which satisfy somewhat less stringent
requirements. Independent confirmation is available for all of these objects,
either from earlier data in the literature or from new observations made with
the Westerbork Synthesis Radio Telescope and reported here. The catalog
includes 54 of the 65 CHVCs listed by Braun and Burton (1999) on the basis of a
visual search of the LDS data.Comment: 17 pages, 19 png/jpeg figures, in review at A&A, (embedded PS figures
removed due to outdated astro-ph size limits
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