Authors: O. Zamora, C. Abia, B. Plez, I. Domínguez and S. Cristallo 
A&A 508, 909 (2009) Received 7 July 2009 / Accepted 17 September 2009
 Keywords: stars: abundances, stars: chemically peculiar, stars: carbon, stars: AGB and post-AGB
Category Archives: Astro Physics
On the origin of reverse polarity patches found by Hinode in sunspot penumbrae
Authors: J. Sánchez Almeida and K. Ichimoto 
A&A 508, 963 (2009) Received 19 May 2009 / Accepted 17 September 2009 
 Keywords: Sun: magnetic fields, Sun: photosphere, sunspots
Flow instabilities of magnetic flux tubes – IV. Flux storage in the solar overshoot region
Authors: E. I??k and V. Holzwarth 
A&A 508, 979 (2009) Received 3 July 2009 / Accepted 22 September 2009 
 Keywords: Sun: interior, Sun: magnetic fields, magnetohydrodynamics (MHD)
A new radiative cooling curve based on an up-to-date plasma emission code
Authors: K. M. Schure, D. Kosenko, J. S. Kaastra, R. Keppens and J. Vink 
A&A 508, 751 (2009) Received 14 May 2009 / Accepted 24 September 2009
 Keywords: hydrodynamics, ISM: evolution, radiation mechanisms: thermal
Fragmentation of a dynamically condensing radiative layer
Authors: K. Iwasaki and T. Tsuribe 
A&A 508, 725 (2009) Received 1 July 2009 / Accepted 14 September 2009 
 Keywords: hydrodynamics, instabilities, ISM: kinematics and dynamics, ISM: structure, ISM: clouds
Wave propagation and energy transport in the magnetic network of the Sun
Authors: G. Vigeesh, S. S. Hasan and O. Steiner 
A&A 508, 951 (2009) Received 8 May 2009 / Accepted 10 September 2009 
 Keywords: Sun: magnetic fields, Sun: photosphere, Sun: faculae, plages, magnetohydrodynamics (MHD), waves
Temporal variations of the CaXIX spectra in solar flares
Authors: R. Falewicz, P. Rudawy and M. Siarkowski 
A&A 508, 971 (2009) Received 29 June 2009 / Accepted 18 September 2009
 Keywords: Sun: chromosphere, Sun: corona, Sun: flares, Sun: magnetic fields, Sun: X-rays, gamma rays
Young T-dwarf candidates in IC 348
Authors: A. S. M. Burgess, E. Moraux, J. Bouvier, C. Marmo, L. Albert and H. Bouy 
A&A 508, 823 (2009) Received 7 May 2009 / Accepted 21 August 2009 
 Keywords: stars: formation, stars: low-mass, brown dwarfs, open clusters and associations: individual: IC 348, stars: luminosity function, mass function, infrared: stars
Deuterium chemistry in the Orion Bar PDR – “Warm” chemistry starring CH_{2}D^+
Authors: B. Parise, S. Leurini, P. Schilke, E. Roueff, S. Thorwirth and D. C. Lis 
A&A 508, 737 (2009) Received 26 June 2009 / Accepted 18 September 2009
 Keywords: astrochemistry, line: identification, line: formation, ISM: abundances, ISM: individual objects: Orion Bar, ISM: molecules
Asteroseismic study of helium and heavy element diffusion in solar-type stars
Authors: N. Gai, S. L. Bi, Y. K. Tang and L. H. Li 
A&A 508, 849 (2009) Received 3 May 2009 / Accepted 18 September 2009 
 Keywords: stars: evolution, stars: interiors, stars: oscillations
Metal abundances in the cool cores of galaxy clusters
Authors: S. De Grandi and S. Molendi 
A&A 508, 565 (2009) Received 22 June 2009 / Accepted 27 August 2009
 Keywords: X-rays: galaxies: clusters, galaxies: clusters: general, supernovae: general, galaxies: abundances, cooling flows, intergalactic medium
A proto brown dwarf candidate in Taurus
Authors: D. Barrado, M. Morales-Calderón, A. Palau, A. Bayo, I. de Gregorio-Monsalvo, C. Eiroa, N. Huélamo, H. Bouy, O. Morata and L. Schmidtobreick 
A&A 508, 859 (2009) Received 4 April 2009 / Accepted 22 September 2009
 Keywords: circumstellar matter, stars: formation, stars: low-mass, brown dwarfs, stars: pre-main sequence, infrared: stars
Revealing the sub-AU asymmetries of the inner dust rim in the disk around the Herbig Ae star R Coronae Austrinae
Authors: S. Kraus, K.-H. Hofmann, F. Malbet, A. Meilland, A. Natta, D. Schertl, P. Stee and G. Weigelt 
A&A 508, 787 (2009) Received 26 July 2009 / Accepted 28 October 2009 
 Keywords: stars: pre-main-sequence, circumstellar matter, accretion, accretion disks, planetary systems: protoplanetary disks, planetary systems: formation, techniques: interferometric
Probing the dust properties of galaxies up to submillimetre wavelengths – I. The spectral energy distribution of dwarf galaxies using LABOCA
Authors: M. Galametz, S. Madden, F. Galliano, S. Hony, F. Schuller, A. Beelen, G. Bendo, M. Sauvage, A. Lundgren and N. Billot 
A&A 508, 645 (2009) Received 23 July 2009 / Accepted 28 September 2009
 Keywords: galaxies: ISM, galaxies: dwarf, infrared: ISM, dust, extinction
On the physical origin of the second solar spectrum of the Sc II line at 4247 Å
Author: L. Belluzzi
A&A 508, 933 (2009) Received 21 July 2009 / Accepted 6 August 2009
 Keywords: atomic processes, polarization, scattering, Sun: atmosphere
Spotting the Minimum
Recently some people have claimed that the Sun
				is entering a new Maunder Minimum—a decades-long period
				of few sunspots—and that this will cause the Earth's
				atmosphere to cool.  The Sun is certainly quiet in 2008,
				but this is the normal quiet of a minimum in the 11 year
				sunspot cycle.  Clearly the tendency to interpret normal
				variations as fundamental changes is not confined to the
				global warming alarmists.
Nuclear Reactions in Thermonuclear Supernovae
Carbon and oxygen are converted into nickel
				in a white dwarf through a complex network of reactions.
				The incremental changes tend to follow the series of atomic
				nuclei that are multiples in composition of the helium
				nucleus.  For this reason, large amounts of neon-20,
				magnesium-24, silicon-28, and other elements with equal
				and even numbers of protons and neutrons are created.  But
				the reactions also tear down nuclei, creating many free
				protons, neutrons, and helium nuclei that combine with
				other atomic nuclei to produce elements and isotopes
				that do not have equal numbers of protons and neutrons
				or do not have an even number of protons or of
				neutrons.  Because thermonuclear fusion disrupts
				a white dwarf, the thermonuclear reactions in
				a white dwarf  contribute to the rich variety
				of chemical elements and isotopes we find throughout
				the universe.
The Structure and Evolution of Brown Dwarfs
The structure of a brown dwarf is set by
				degeneracy pressure.  Unlike a star, where the mass
				sets both the radius and the photospheric temperature,
				a brown dwarf has a radius and temperature that is nearly
				independent of its mass.  All brown dwarfs are about
				the same size as Jupiter.  The photospheric temperature
				of a brown dwarf is set by its age, although the lifetime
				of a brown dwarf is set by the mass.  Because the
				low-mass brown dwarfs cool much faster than the
				high-mass brown dwarfs, infrared surveys preferentially
				find the more-massive brown dwarfs.
Core-Collapse Supernovae
The most energetic supernovae are powered by gravitational potential energy.
				Once a massive star consumes all of its thermonuclear fuel, it is unable to support
				itself against its own gravity.  The core of such a star collapses to a neutron star.
				The birth of a neutron star is heralded by a burst of neutrinos that blows apart
				the remainder of the star.  We see this expanding debris as a supernova.
No Bang from the Big Bang Machine
The Large Hadron Collider at CERN, a machine
				that accelerates protons to very high energies and then
				bangs them together, began operating on September 10, 2008.
				Some believe this machine threatens Earth. They need not
				worry, because the particle collisions created in this
				machine occur daily when cosmic rays strike Earth's
				atmosphere. Man can't yet rival nature's extremes.
