34,440 research outputs found
Giant star seismology
The internal properties of stars in the red-giant phase undergo significant
changes on relatively short timescales. Long near-uninterrupted high-precision
photometric timeseries observations from dedicated space missions such as CoRoT
and Kepler have provided seismic inferences of the global and internal
properties of a large number of evolved stars, including red giants. These
inferences are confronted with predictions from theoretical models to improve
our understanding of stellar structure and evolution. Our knowledge and
understanding of red giants have indeed increased tremendously using these
seismic inferences, and we anticipate that more information is still hidden in
the data. Unraveling this will further improve our understanding of stellar
evolution. This will also have significant impact on our knowledge of the Milky
Way Galaxy as well as on exo-planet host stars. The latter is important for our
understanding of the formation and structure of planetary systems.Comment: Invited review for The Astronomy and Astrophysics Review, accepted
for publicatio
On the choice of parameters in solar structure inversion
The observed solar p-mode frequencies provide a powerful diagnostic of the
internal structure of the Sun and permit us to test in considerable detail the
physics used in the theory of stellar structure. Amongst the most commonly used
techniques for inverting such helioseismic data are two implementations of the
optimally localized averages (OLA) method, namely the Subtractive Optimally
Localized Averages (SOLA) and Multiplicative Optimally Localized Averages
(MOLA). Both are controlled by a number of parameters, the proper choice of
which is very important for a reliable inference of the solar internal
structure. Here we make a detailed analysis of the influence of each parameter
on the solution and indicate how to arrive at an optimal set of parameters for
a given data set.Comment: 14 pages, 15 figures. Accepted for publication on MNRA
Observations of the 1992 U.S. Pelagic Pair Trawl Fishery in the Northwest Atlantic
Pelagic pair trawling for tuna, Thunnus spp., and swordfish, Xiphias gladius, was introduced in U.S. Northwest Atlantic waters in 1991. During autumn (October-November) of 1992 under the authority oft he Federal Atlantic Swordfish Regulations, the National Marine Fisheries Service placed observers aboard pelagic pair trawl vessels to document the catch, bycatch, discard, and gear used in this new fishery. The fishery is conducted primarily at night along shelf-edge waters from June to November. In late 1991, revised regulations restricted swordfish to bycatch in this fishery resulting in pelagic pair trawl vessels targeting tuna throughout 1992. Analyses of 1992 data indicate that albacore, T. alalunga, was the predominant species caught, although yellowfin tuna,
T. albaeares, and bigeye tuna, T. obesus, were the preferred target species. Bycatch also included swordfish, large sharks, pelagic rays and other pelagic fishes, other tunas, and marine mammals
The concept of social pharmacy
The 13th International Social Pharmacy Workshop will be held in Malta in July 2004. The Social Pharmacy Workshops are international conferences for research in social and behavioural pharmacy. Meetings are held every second year and participation has grown steadily since the first Workshop was held in Helsinki, Finland, in 1980. Following the successful 2002 conference in Sydney, Australia, the 2004 meeting in Malta will be the first one held in the Mediterranean area!peer-reviewe
On the asymptotic acoustic-mode phase in red-giant stars and its dependence on evolutionary state
Asteroseismic investigations based on the wealth of data now available,in
particular from the CoRoT and Kepler missions, require a good understanding of
the relation between the observed quantities and the properties of the
underlying stellar structure. Kallinger et al. 2012 found a relation between
their determination of the asymptotic phase of radial oscillations in evolved
stars and the evolutionary state, separating ascending-branch red giants from
helium-burning stars in the `red clump'. Here we provide a detailed analysis of
this relation, which is found to derive from differences between these two
classes of stars in the thermodynamic state of the convective envelope. There
is potential for distinguishing red giants and clump stars based on the phase
determined from observations that are too short to allow distinction based on
determination of the period spacing for mixed modes. The analysis of the phase
may also point to a better understanding of the potential for using the
helium-ionization-induced acoustic glitch to determine the helium abundance in
the envelopes of these stars.Comment: MNRAS, in the pres
Stellar Oscillations Network Group
Stellar Oscillations Network Group (SONG) is an initiative aimed at designing
and building a network of 1m-class telescopes dedicated to asteroseismology and
planet hunting. SONG will have 8 identical telescope nodes each equipped with a
high-resolution spectrograph and an iodine cell for obtaining precision radial
velocities and a CCD camera for guiding and imaging purposes. The main
asteroseismology targets for the network are the brightest (V<6) stars. In
order to improve performance and reduce maintenance costs the instrumentation
will only have very few modes of operation. In this contribution we describe
the motivations for establishing a network, the basic outline of SONG and the
expected performance.Comment: Proc. Vienna Workshop on the Future of Asteroseismology, 20 - 22
September 2006. Comm. in Asteroseismology, Vol. 150, in the pres
- …