4,563 research outputs found
The Generation of Fullerenes
We describe an efficient new algorithm for the generation of fullerenes. Our
implementation of this algorithm is more than 3.5 times faster than the
previously fastest generator for fullerenes -- fullgen -- and the first program
since fullgen to be useful for more than 100 vertices. We also note a
programming error in fullgen that caused problems for 136 or more vertices. We
tabulate the numbers of fullerenes and IPR fullerenes up to 400 vertices. We
also check up to 316 vertices a conjecture of Barnette that cubic planar graphs
with maximum face size 6 are hamiltonian and verify that the smallest
counterexample to the spiral conjecture has 380 vertices.Comment: 21 pages; added a not
Prospects for CW and LP operation of the European XFEL in hard X-ray regime
The European XFEL will operate nominally at 17.5 GeV in SP (short pulse) mode
with 0.65 ms long bunch train and 10 Hz repetition rate. A possible upgrade of
the linac to CW (continuous wave) or LP (long pulse) modes with a corresponding
reduction of electron beam energy is under discussion since many years. Recent
successes in the dedicated R&D program allow to forecast a technical
feasibility of such an upgrade in the foreseeable future. One of the challenges
is to provide sub-Angstrom FEL operation in CW and LP modes. In this paper we
perform a preliminary analysis of a possible operation of the European XFEL in
the hard X-ray regime in CW and LP modes with the energies of 7 GeV and 10 GeV,
respectively. We consider lasing in the baseline XFEL undulator as well as in a
new undulator with a reduced period. We show that, with reasonable requirements
on electron beam quality, lasing on the fundamental will be possible in
sub-Angstrom regime. As an option for generation of brilliant photon beams at
short wavelengths we also consider harmonic lasing that has recently attracted
a significant attention
Synthetic X-ray light curves of BL Lacs from relativistic hydrodynamic simulations
We present the results of relativistic hydrodynamic simulations of the
collision of two dense shells in a uniform external medium, as envisaged in the
internal shock model for BL Lac jets. The non-thermal radiation produced by
highly energetic electrons injected at the relativistic shocks is computed
following their temporal and spatial evolution. The acceleration of electrons
at the relativistic shocks is parametrized using two different models and the
corresponding X-ray light curves are computed. We find that the interaction
time scale of the two shells is influenced by an interaction with the external
medium. For the chosen parameter sets, the efficiency of the collision in
converting dissipated kinetic energy into the observed X-ray radiation is of
the order of one percent.Comment: 22 pages, 6 figures, accepted to A&
Radio-loud Active Galaxies in the Northern ROSAT All-Sky Survey III: New Spectroscopic Identifications from the RGB BL Lac Survey
We present new spectroscopic identifications for 169 objects in the
RASS-Green Bank (RGB) catalog of radio- and X-ray-emitting AGN. These data
significantly increase the fraction of bright RGB objects with classifications.
Specifically, we report and discuss the classification of 66 radio-loud
quasars, 53 BL Lacs, 33 Broad Line Radio Galaxies, 5 Narrow Line Radio
Galaxies, 1 Seyfert I galaxy and 11 galaxies or galaxies in clusters. Over 78%
of the identifications we present here are new. The observations we report were
undertaken as part of our targeted search program to identify a new, large
unbiased sample of BL Lac Objects and we therefore discuss the BL Lac sample
extensively. Unlike many previous surveys, we impose no selection criteria
based on optical morphology, color or broadband spectral energy distribution.
Our classifications are based solely on a carefully defined set of
self-consistent spectroscopic classification criteria. We show the 53 RGB
presented here exhibit transitional properties between normal galaxies and BL
Lacs discovered previously. We show there is no clear separation in CaII break
strength between RGB BL Lacs and galaxies, with the distribution of break
strengths varying smoothly between 0% and 50%. We also show that the newly
discovered RGB BL Lacs reside in a "zone of avoidance" in the log(S_x/S_r) vs.
log(S_o/S_r) diagram. This has important implications for BL Lac search
strategies since it shows that RASS BL Lac samples will be severely incomplete
if candidates are chosen only from among those objects with the highest S_x/S_r
flux ratios.Comment: 21 pages text, 189 Figures, 4 tables, LaTeX2E, 4.2MB tar file
(compressed); special style file paper.sty provide
Detection of a high frequency break in the X-ray power spectrum of Ark 564
We present a power spectrum analysis of the long ASCA observation of Ark 564
in June/July 2001. The observed power spectrum covers a frequency range of ~
3.5 decades. We detect a high frequency break at ~ 0.002 Hz. The power spectrum
has an rms of ~30% and a slope of ~ -1 and ~ -2 below and above the break
frequency. When combined with the results from a long RXTE observation (Pounds
et al. 2001), the observed power spectra of Ark 564 and Cyg X-1 (in the
low/hard state) are almost identical, showing a similar shape and rms
amplitude. However, the ratio of the high frequency breaks is very small (~
10e{3-4}), implying that these characteristic frequencies are not indicative of
the black hole mass. This result supports the idea of a small black hole
mass/high accretion rate in Ark 564.Comment: 4 pages, 3 figures, A&A (Letters) in pres
Revisiting algorithms for generating surrogate time series
The method of surrogates is one of the key concepts of nonlinear data
analysis. Here, we demonstrate that commonly used algorithms for generating
surrogates often fail to generate truly linear time series. Rather, they create
surrogate realizations with Fourier phase correlations leading to
non-detections of nonlinearities. We argue that reliable surrogates can only be
generated, if one tests separately for static and dynamic nonlinearities.Comment: 5 pages, 4 figures, accepted for publication in PR
RBSC-NVSS Sample. I. Radio and Optical Identifications of a Complete Sample of 1500 Bright X-ray Sources
We cross-identified the ROSAT Bright Source Catalog (RBSC) and the NRAO VLA
Sky Survey (NVSS) to construct the RBSC-NVSS sample of the brightest X-ray
sources (>= 0.1 counts/s or ~1E-12 ergs/cm/cm/s in the 0.1-2.4 keV band) that
are also radio sources (S >= 2.5 mJy at 1.4 GHz) in the 7.8 sr of extragalactic
sky with |b| > 15 degrees. and delta > -40 degrees. The sky density of NVSS
sources is low enough that they can be reliably identified with RBSC sources
having average rms positional uncertainties = 10 arcsec. We used the more
accurate radio positions to make reliable X-ray/radio/optical identifications
down to the POSS plate limits. We obtained optical spectra for many of the
bright identifications lacking published redshifts. The resulting X-ray/radio
sample is unique in its size (N ~ 1500 objects), composition (a mixture of
nearly normal galaxies, Seyfert galaxies, quasars, and clusters), and low
average redshift ( ~ 0.1).Comment: 35 LaTeX pages including 6 eps figures + 40 LaTeX page table2
(landscape) w/ AASTeX 5.0; accepted to ApJ
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