1,374 research outputs found
Curious Variables Experiment (CURVE). CCD photometry of active dwarf nova DI UMa
We report an analysis of photometric behaviour of DI UMa, an extremely active
dwarf nova. The observational campaign (completed in 2007) covers five
superoutbursts and four normal outbursts. We examined principal parameters of
the system to understand peculiarities of DI UMa, and other active cataclysmic
variables. Based on precise photometric measurements, temporal light curve
behaviour, O-C analysis, and power spectrum analysis, we investigated physical
parameters of the system. We found that the period of the supercycle now equals
31.45 +/-0.3 days. Observations during superoutbursts infer that the period of
superhumps equals P_sh = 0.055318(11) days (79.66 +/- 0.02 min). During
quiescence, the light curve reveals a modulation of period P_orb = 0.054579(6)
days (78.59 +/- 0.01 min), which we interpret as the orbital period of the
binary system. The values obtained allowed us to determine a fractional period
excess of 1.35% +/- 0.02%, which is surprisingly small compared to the usual
value for dwarf novae (2%-5%). A detailed O-C analysis was performed for two
superoutbursts with the most comprehensive coverage. In both cases, we detected
an increase in the superhump period with a mean rate of dot_P/P_sh =
4.4(1.0)*10^{-5}. Based on these measurements, we confirm that DI UMa is
probably a period bouncer, an old system that reached its period minimum a long
time ago, has a secondary that became a degenerate brown dwarf, the entire
system evolving now toward longer periods. DI UMa is an extremely interesting
object because we know only one more active ER UMa star with similar
characteristics (IX Dra).Comment: Accepted for publication in Astronomy & Astrophysic
In-the-Gap SU UMa-Type Dwarf Nova, Var73 Dra with a Supercycle of about 60 Days
An intensive photometric-observation campaign of the recently discovered SU
UMa-type dwarf nova, Var73 Dra was conducted from 2002 August to 2003 February.
We caught three superoutbursts in 2002 October, December and 2003 February. The
recurrence cycle of the superoutburst (supercycle) is indicated to be 60
d, the shortest among the values known so far in SU UMa stars and close to
those of ER UMa stars. The superhump periods measured during the first two
superoutbursts were 0.104885(93) d, and 0.10623(16) d, respectively. A
0.10424(3)-d periodicity was detected in quiescence. The change rate of the
superhump period during the second superoutburst was , which
is an order of magnitude larger than the largest value ever known. Outburst
activity has changed from a phase of frequent normal outbursts and infrequent
superoutbursts in 2001 to a phase of infrequent normal outbursts and frequent
superoutbursts in 2002. Our observations are negative to an idea that this star
is an related object to ER UMa stars in terms of the duty cycle of the
superoutburst and the recurrence cycle of the normal outburst. However, to
trace the superhump evolution throughout a superoutburst, and from quiescence
more effectively, may give a fruitful result on this matter.Comment: 9 pages, 8 figures, submitted to A&
Realization of a collective decoding of codeword states
This was also extended from the previous article quant-ph/9705043, especially
in a realization of the decoding process.Comment: 6 pages, RevTeX, 4 figures(EPS
Is CSR a magic word?: An exploring study of consumer behaviour in cosmetic market in Thailand
Many authors stated that decision-making today is more complex than in the past, especially when they are being confronted by various kinds of product (eg.: Hafstrom et al., 1992; Lysonski et al., 1995; Mitchell et al., 1998). Thailand is an example of a developing country where a huge number of products from various countries imported cosmetic products. Due to the competition in Thailand, cosmetic market is always very intense; therefore it is important for firms to understand the factors that affect the consumers purchasing behaviour. At the same time, Corporate Social Responsibility (CSR) has been one of the most popular theme for academics and marketers when they analyse its impact on consumers’ behaviour (Maignan and Ferrel, 2004; Smith, 2003). Does CSR have a positive impact on Thai consumers’ purchasing intention? To investigate this theme based on quantitative approach, we analyse the impact of CSR factor as an antecedent factor for Thai consumers’ attitudes towards cosmetic products, drawing the pathways resulting in their final decision of purchasing
Accessible information and optimal strategies for real symmetrical quantum sources
We study the problem of optimizing the Shannon mutual information for sources
of real quantum states i.e. sources for which there is a basis in which all the
states have only real components. We consider in detail the sources of equiprobable qubit states lying symmetrically around the great
circle of real states on the Bloch sphere and give a variety of explicit
optimal strategies. We also consider general real group-covariant sources for
which the group acts irreducibly on the subset of all real states and prove the
existence of a real group-covariant optimal strategy, extending a theorem of
Davies (E. B. Davies, IEEE. Inf. Theory {\bf IT-24}, 596 (1978)). Finally we
propose an optical scheme to implement our optimal strategies, enough simple to
be realized with present technology.Comment: RevTeX, 16 pages, 4 eps figures with psfig, submitted to Phys. Rev.
A, corrected output error of Fig. 1 in the previous versio
The fractional Keller-Segel model
The Keller-Segel model is a system of partial differential equations
modelling chemotactic aggregation in cellular systems. This model has blowing
up solutions for large enough initial conditions in dimensions d >= 2, but all
the solutions are regular in one dimension; a mathematical fact that crucially
affects the patterns that can form in the biological system. One of the
strongest assumptions of the Keller-Segel model is the diffusive character of
the cellular motion, known to be false in many situations. We extend this model
to such situations in which the cellular dispersal is better modelled by a
fractional operator. We analyze this fractional Keller-Segel model and find
that all solutions are again globally bounded in time in one dimension. This
fact shows the robustness of the main biological conclusions obtained from the
Keller-Segel model
An Irradiation Effect in Nova DN Gem 1912 and the Significance of the Period Gap for Classical Novae
Continuous CCD photometry of the classical nova DN Gem during 52 nights in
the years 1992-98 reveals a modulation with a period 0.127844 d. The
semi-amplitude is about 0.03 mag. The stability of the variation suggests that
it is the orbital period of the binary system. This interpretation makes DN Gem
the fourth nova inside the cataclysmic variable (CV) period gap, as defined by
Diaz and Bruch (1997), and it bolsters the idea that there is no period gap for
classical novae. However, the number of known nova periods is still too small
to establish this idea statistically. We eliminate several possible mechanisms
for the variation, and propose that the modulation is driven by an irradiation
effect. We find that model light curves of an irradiated secondary star, fit
the data well. The inclination angle of the system is restricted by this model
to 10 deg < i < 65 deg. We also refine a previous estimate of the distance to
the binary system, and find d=1.6+/-0.6 kpc.Comment: 7 pages, Latex file, 2 .ps files and 3 .eps files. accepted for
publication in MNRAS. also available at:
ftp://ftp.astro.keele.ac.uk/pub/preprints/preprints.htm
Dipolar modes in luminous red giants
Lots of information on solar-like oscillations in red giants has been
obtained thanks to observations with CoRoT and Kepler space telescopes. Data on
dipolar modes appear most interesting. We study properties of dipolar
oscillations in luminous red giants to explain mechanism of mode trapping in
the convective envelope and to assess what may be learned from the new data.
Equations for adiabatic oscillations are solved by numerical integration down
to the bottom of convective envelope, where the boundary condition is applied.
The condition is based on asymptotic decomposition of the fourth order system
into components describing a running wave and a uniform shift of radiative
core. If the luminosity of a red giant is sufficiently high, for instance at M
= 2 Msun greater than about 100 Lsun, the dipolar modes become effectively
trapped in the acoustic cavity, which covers the outer part of convective
envelope. Energy loss caused by gravity wave emission at the envelope base is a
secondary or negligible source of damping. Frequencies are insensitive to
structure of the deep interior.Comment: 10 pages, 7 figures, accepted for publication in Astronomy and
Astrophysic
The one-dimensional Keller-Segel model with fractional diffusion of cells
We investigate the one-dimensional Keller-Segel model where the diffusion is
replaced by a non-local operator, namely the fractional diffusion with exponent
. We prove some features related to the classical
two-dimensional Keller-Segel system: blow-up may or may not occur depending on
the initial data. More precisely a singularity appears in finite time when
and the initial configuration of cells is sufficiently concentrated.
On the opposite, global existence holds true for if the initial
density is small enough in the sense of the norm.Comment: 12 page
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