Search Publications

A low luminosity state in the massive X-ray binary SAX J0635+0533
DOI: 10.1051/0004-6361/200911944 Bibcode: 2009A&A...504..181M

Mereghetti, S.; La Palombara, N.

The X-ray pulsar SAX J0635+0533 was repeatedly observed with the XMM-Newton satellite in 2003-2004. The precise localization provided by these observations confirms the association of SAX J0635+0533 with a Be star. The source was found, for the first time, in a low-intensity state, a factor ~30 lower than that seen in all previous observations. Th…

2009 Astronomy and Astrophysics
XMM-Newton 2
The evolution of cluster dwarfs
DOI: 10.1002/asna.200911269 Bibcode: 2009AN....330..937H

Harsono, D.; De Propris, R.

We summarize the results from analyzing six clusters of galaxies at 0.14 < z < 0.40 observed with the Hubble Space Telescope Advanced Camera for Surveys. We derive deep composite luminosity functions in B, g, V, r, i, and z down to absolute magnitude of ∼ -14 + 5 log h mag. The luminosity functions are fitted by a single Schechter function w…

2009 Astronomische Nachrichten
eHST 2
Fresnel zone plate telescopes for X-ray imaging II: numerical simulations with parallel and diverging beams
DOI: 10.1007/s10686-009-9176-3 Bibcode: 2009ExA....27...77P

Rao, A. R.; Girish, V.; Nandi, Anuj +4 more

We present the results of simulations of shadows cast by a zone plate telescope which may have one to four pairs of zone plates. From the shadows we reconstruct the images under various circumstances. We discuss physical basis of the resolution of the telescope and demonstrate this by our simulations. We allow the source to be at a finite distance…

2009 Experimental Astronomy
INTEGRAL 2
On the predictability of unstable satellite motion around elongated celestial bodies
DOI: 10.1051/0004-6361/200811279 Bibcode: 2009A&A...506..989M

Mysen, E.

Context: Close satellite orbits around small and elongated celestial bodies can experience massive aperiodic changes in shape. According to a number of published works, the changes are continuous functions of the orbit elements of the satellite's unperturbed trajectory.
Aims: Later research, however, has revealed that the onset of instability …

2009 Astronomy and Astrophysics
Rosetta 2
Spatial and Spectral Behaviors of Solar Flares Observed in Microwaves
DOI: 10.1007/s11207-009-9388-8 Bibcode: 2009SoPh..257..335N

Cao, Wenda; Ning, Zongjun

The spatial and spectral behaviors of two solar flares observed by the Nobeyama Radioheliograph (NoRH) on 24 August 2002 and 22 August 2005 are explored. They were observed with a single loop-top source and double footpoint sources at the beginning, then with looplike structures for the rest of the event. NoRH has high spatial and temporal resolut…

2009 Solar Physics
SOHO 2
Space projections on solar-terrestrial physics
DOI: 10.1134/S0016793209080209 Bibcode: 2009Ge&Ae..49.1137K

Zelenyi, L. M.; Kuznetsov, V. D.

An overview of the current status of research in the field of solar-terrestrial physics conducted by space agencies of various countries is given. The main results of current (Ulysses, SOHO, TRACE, RHESSI, Hinode, and STEREO) and completed (Coronas-F and others) missions as well as the scientific goals and objectives of space projects being prepar…

2009 Geomagnetism and Aeronomy
Ulysses 2
Reconnection Hall current system observed in the magnetotail and in the ionosphere
DOI: 10.1029/2009GL037239 Bibcode: 2009GeoRL..36.8104S

Snekvik, K.; Østgaard, N.; Amm, O. +1 more

On 07 Sep 2001 around 21:40 UT, Cluster was located 19 R E downtail, and observed earthward fast flows and strong perturbations in the dawn-dusk component of the magnetic field (B Y ). The perturbations corresponded to a sheet of tailward field aligned current close to the neutral sheet and another sheet of earthward field…

2009 Geophysical Research Letters
Cluster 2
A Repository of Precision Flat Fields for High-Resolution MDI Continuum Data
DOI: 10.1007/s11207-009-9408-8 Bibcode: 2009SoPh..258..343P

Potts, H. E.; Diver, D. A.

We describe an archive of high-precision MDI flat fields that can be used to refine most MDI high-resolution continuum data. The archive consists of many flat-field images representing different time ranges over the full operating period of SOHO. The residual flat-field error on the standard level 1.5/1.8 calibrated continuum images represents a s…

2009 Solar Physics
SOHO 2
Diffuse 18µ Emission around TYC 3159-6-1 Discovered by the AKARI MIR All-Sky Survey
DOI: 10.1093/pasj/61.2.291 Bibcode: 2009PASJ...61..291T

Oyabu, Shinki; Onaka, Takashi; Takita, Satoshi +11 more

We report on observations of the mysterious object TYC 3159-6-1 located toward the Cygnus X region. It shows interesting characteristics in the AKARI mid-infrared All-Sky Survey. The central star is clearly detected as a point source at 9µ, while no point-like source, but a large shell-like structure is seen around the source at 18µ. T…

2009 Publications of the Astronomical Society of Japan
AKARI 2
Erratum: "Suzaku Observations of Local Ultraluminous Infrared Galaxies" (2009, ApJ, 691, 261)
DOI: 10.1088/0004-637X/701/2/2035 Bibcode: 2009ApJ...701.2035T

Sanders, D. B.; Nakagawa, Takao; Veilleux, Sylvain +7 more

We report the results from our analysis of {\it Suzaku} XIS (0.5-10 keV) and HXD/PIN (15-40 keV) observations of five well-known local ULIRGs: {\em IRAS} F05189-2524, {\em IRAS} F08572+3915, Mrk 273, PKS 1345+12, and Arp 220. The XIS observations of F05189-2524 and Mrk 273 reveal strong iron lines consistent with Fe K$\alpha$ and changes in spectr…

2009 The Astrophysical Journal
Suzaku 2