267 research outputs found
UKIRT follow-up observations of the old open cluster FSR0358 (Kirkpatrick1)
We aim to characterise the properties of the stellar clusters in the Milky
Way. Utilising an expectation-maximisation method we determined that the
cluster FSR0358, originally discovered by J.D.Kirkpatrick, is the most likely
real cluster amongst the cluster candidates from Froebrich et al.. Here we
present new deep high resolution near infrared imaging of this object obtained
with UKIRT. The analysis of the data reveals that FSR0358 (Kirkpatrick1) is a
5+-2Gyr old open cluster in the outer Milky Way. Its age, metallicity of
Z=0.008 and distance from the Galactic Centre of 11.2kpc are typical for the
known old open galactic clusters. So far six of the FSR cluster candidates have
been identified as having an age above 5Gyr. This shows the significance of
this catalogue in enhancing our knowledge of the oldest open clusters in the
Galaxy.Comment: 8 pages, 1 table, 5 figures, accepted for publication by MNRAS, a
version with higher resolution figures can be found at
http://astro.kent.ac.uk/~df
A near-infrared variability study in the cloud IC1396W: low star-forming efficiency and two new eclipsing binaries
Identifying the population of young stellar objects (YSOs) in high extinction
regions is a prerequisite for studies of star formation. This task is not
trivial, as reddened background objects can be indistinguishable from YSOs in
near-infrared colour-colour diagrams. Here we combine deep JHK photometry with
J- and K-band lightcurves, obtained with UKIRT/WFCAM, to explore the YSO
population in the dark cloud IC1396W. We demonstrate that a colour-variability
criterion can provide useful constraints on the star forming activity in
embedded regions. For IC1396W we find that a near-infrared colour analysis
alone vastly overestimates the number of YSOs. In total, the globule probably
harbours not more than ten YSOs, among them a system of two young stars
embedded in a small (~10000 AU) reflection nebula. This translates into a star
forming efficiency SFE of ~1%, which is low compared with nearby more massive
star forming regions, but similar to less massive globules. We confirm that
IC1396W is likely associated with the IC1396 HII region. One possible
explanation for the low SFE is the relatively large distance to the ionizing
O-star in the central part of IC1396. Serendipitously, our variability campaign
yields two new eclipsing binaries, and eight periodic variables, most of them
with the characteristics of contact binaries.Comment: 13 pages, 10 figures, MNRAS, in pres
Oplossingen voor landbouw in Noord-Afrika
In Egypte en de Maghreb-landen kijken onderzoekers van Alterra naar mogelijkheden voor landbouwontwikkeling, ondanks schaarste aan goed water en landbouwgrond. Mogelijk liggen er kansen voor het Nederlandse bedrijfsleven
Many-body Green's function theory for thin ferromagnetic films: exact treatment of the single-ion anisotropy
A theory for the magnetization of ferromagnetic films is formulated within
the framework of many-body Green's funtion theory which considers all
components of the magnetization. The model Hamiltonian includes a Heisenberg
term, an external field, a second- and fourth-order uniaxial single-ion
anisotropy, and the magnetic dipole-dipole coupling. The single-ion anisotropy
terms can be treated exactly by introducing higher-order Green's functions and
subsequently taking advantage of relations between products of spin operators
which leads to an automatic closure of the hierarchy of the equations of motion
for the Green's functions with respect to the anisotropy terms. This is an
improvement on the method of our previous work, which treated the corresponding
terms only approximately by decoupling them at the level of the lowest-order
Green's functions. RPA-like approximations are used to decouple the exchange
terms in both the low-order and higher-order Green's functions. As a first
numerical example we apply the theory to a monolayer for spin S=1 in order to
demonstrate the superiority of the present treatment of the anisotropy terms
over the previous approximate decouplings.Comment: 23 pages, 5 figure
Applicability of adapted reservoir operation for water stress mitigation under dry year conditions
This paper introduces the conjunctive use of a deterministic water quality model and water balance criteria for supporting the assessment of simulation and to evaluate the effectiveness of proposed operation strategies. By this, the applicability of enhanced reservoir operation strategies addressing both water quality as well as water quantity aspects under water deficit conditions in dry years can be shown. Arguments will be developed to address stakeholders and decision makers in the context of a more conservative past operation regime. Results are presented for the Kaparas reservoir, which is located in the lower Amu Darya River, on the border of Turkmenistan and Uzbekistan. As being one out of four large reservoirs of the Tuyamuyun Hydro Complex (THC), the Kaparas reservoir could be increasingly used for drinking water supply for the lower Amu Darya region. The results for the dry year 2001 indicates that the combination of simulation together with practical assessment criteria confirm the applicability of adapted operation rules for THC reservoirs and ways can be found to supply the local population (of the lower Amu Darya region) with more potable water of higher quality even subject to a parallel reduction of water deficits. Future aggravation of water stress due to increasing population growth and water quality deterioration will require a more comprehensive consideration of water quality aspects in many arid and semi arid regions. The experience gained during this study emphasizes the fact that classical deterministic water quality models provide effective tools to address even more complex water quality problems under water stressed conditions, provided processing of results is performed, to support the decision making process
A large scale extinction map of the Galactic Anticenter from 2MASS
We present a 127deg x 63deg extinction map of the Anticenter of the Galaxy,
based on and colour excess maps from 2MASS. This 8001 square degree
map with a resolution of 4 arcminutes is provided as online material. The
colour excess ratio / is used to determine the power law index of
the reddening law (\beta) for individual regions contained in the area (e.g.
Orion, Perseus, Taurus, Auriga, Monoceros, Camelopardalis, Cassiopeia). On
average we find a dominant value of \beta=1.8+-0.2 for the individual clouds,
in agreement with the canonical value for the interstellar medium. We also show
that there is an internal scatter of \beta values in these regions, and that in
some areas more than one dominant \beta value is present. This indicates large
scale variations in the dust properties. The analysis of the A_V values within
individual regions shows a change in the slope of the column density
distribution with distance. This can either be attributed to a change in the
governing physical processes in molecular clouds on spatial scales of about 1pc
or an A_V dilution with distance in our map.Comment: 18 pages, 29 Figures, 1 Table, Accepted for publication by MNRAS, A
version with higher resolution figures can be found at
http://astro.kent.ac.uk/~df
Characterizing temporary hydrological regimes at a European scale
Monthly duration curves have been constructed from climate data across Europe to help address the relative frequency of ecologically critical low flow stages in temporary rivers, when flow persists only in disconnected pools in the river bed. The hydrological model is 5 based on a partitioning of precipitation to estimate water available for evapotranspiration and plant growth and for residual runoff. The duration curve for monthly flows has then been analysed to give an estimate of bankfull flow based on recurrence interval. The corresponding frequency for pools is then based on the ratio of bank full discharge to pool flow, arguing from observed ratios of cross-sectional areas at flood 10 and low flows to estimate pool flow as 0.1% of bankfull flow, and so estimate the frequency of the pool conditions that constrain survival of river-dwelling arthropods and fish. The methodology has been applied across Europe at 15 km resolution, and can equally be applied under future climatic scenarios
Developing a novel approach to analyse the regimes of temporary streams and their controls on aquatic biota
Temporary streams are those water courses that undergo the recurrent cessation of flow or the complete drying of their channel. The biological communities in temporary stream reaches are strongly dependent on the temporal changes of the aquatic habitats determined by the hydrological conditions. The use of the aquatic fauna structural and functional characteristics to assess the ecological quality of a temporary stream reach can not therefore be made without taking into account the controls imposed by the hydrological regime. This paper develops some methods for analysing temporary streams' aquatic regimes, based on the definition of six aquatic states that summarize the sets of mesohabitats occurring on a given reach at a particular moment, depending on the hydrological conditions: flood, riffles, connected, pools, dry and arid. We used the water discharge records from gauging stations or simulations using rainfall-runoff models to infer the temporal patterns of occurrence of these states using the developed aquatic states frequency graph. The visual analysis of this graph is complemented by the development of two metrics based on the permanence of flow and the seasonal predictability of zero flow periods. Finally, a classification of the aquatic regimes of temporary streams in terms of their influence over the development of aquatic life is put forward, defining Permanent, Temporary-pools, Temporary-dry and Episodic regime types. All these methods were tested with data from eight temporary streams around the Mediterranean from MIRAGE project and its application was a precondition to assess the ecological quality of these streams using the current methods prescribed in the European Water Framework Directive for macroinvertebrate communities
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