Search Publications

Detailed radio to soft γ-ray studies of the 2005 outburst of the new X-ray transient XTE J1818-245
DOI: 10.1051/0004-6361/200810744 Bibcode: 2009A&A...501....1C

D'Avanzo, P.; Campana, S.; Goldoni, P. +11 more

Context: XTE J1818-245 is an X-ray nova that experienced an outburst in 2005, as first seen by the <sl>RXTE</sl> satellite. The source was observed simultaneously at various wavelengths up to soft γ-rays with the <sl>INTEGRAL</sl> satellite, from 2005 February to September, during our <sl>INTEGRAL</sl> Target of…

2009 Astronomy and Astrophysics
INTEGRAL 22
The AGN nature of three INTEGRAL sources: IGR J18249-3243, IGR J19443+2117, and IGR J22292+6647
DOI: 10.1051/0004-6361:200810503 Bibcode: 2009A&A...493..893L

Masetti, N.; Gehrels, N.; Capitanio, F. +6 more

Context: The third INTEGRAL/IBIS survey has revealed several new hard X-ray sources, which are still unidentified or unclassified. To identify these sources, we need to find their counterparts at other wavelengths and then study their nature.
Aims: The aim of this work is to employ the capability of the X-ray telescope (XRT) onboard Swift to l…

2009 Astronomy and Astrophysics
INTEGRAL XMM-Newton 22
Radial Velocity Search for Extrasolar Planets in Visual Binary Systems
DOI: 10.1093/pasj/61.1.19 Bibcode: 2009PASJ...61...19T

Sato, Bun'ei; Itoh, Yoichi; Oasa, Yumiko +7 more

We searched for extrasolar planets in visual binary systems using precise Doppler-shift measurements taken over a period of 4 yr. Using the HIgh Dispersion Echelle Spectrograph (HIDES) equipped on the Okayama Astrophysical Observatory (OAO) 188cm reflector, we achieved a radial-velocity precision of about 10ms-1. We monitored both prima…

2009 Publications of the Astronomical Society of Japan
Hipparcos 21
Comparative clustering analysis of variable stars in the Hipparcos, OGLE Large Magellanic Cloud, and CoRoT exoplanet databases
DOI: 10.1051/0004-6361/200912009 Bibcode: 2009A&A...506..535S

Sarro, L. M.; Aerts, C.; Debosscher, J. +1 more

Context: Discovery of new variability classes in large surveys using multivariate statistics techniques such as clustering, relies heavily on the correct understanding of the distribution of known classes as point processes in parameter space.
Aims: Our objective is to analyze the correspondence between the classical stellar variability types …

2009 Astronomy and Astrophysics
Hipparcos 21
The change of magnetic inclination angles associated with the X3.4 flare on December 13, 2006
DOI: 10.1007/s11433-009-0238-3 Bibcode: 2009ScChG..52.1702L

Jing, Ju; Wang, Haimin; Tan, Changyi +1 more

Recent studies showed a consistent pattern of changes in the sunspot structure associated with major flares: part of the peripheral penumbral regions vanishes during flares, and meanwhile, the umbral cores and/or inner penumbral regions are darkened. To understand the underlying physics of these observations, we compare the magnetic inclination an…

2009 Science in China: Physics, Mechanics and Astronomy
Hinode 21
V3885 Sagittarius: A Comparison with a Range of Standard Model Accretion Disks
DOI: 10.1088/0004-637X/703/2/1839 Bibcode: 2009ApJ...703.1839L

Szkody, Paula; Sion, Edward M.; Godon, Patrick +3 more

A \widetilde{χ}^2 analysis of standard model accretion disk synthetic spectrum fits to combined Far Ultraviolet Spectroscopic Explorer and Space Telescope Imaging Spectrograph spectra of V3885 Sagittarius, on an absolute flux basis, selects a model that accurately represents the observed spectral energy distribution. Calculation of the synthetic s…

2009 The Astrophysical Journal
Hipparcos eHST 21
Radio continuum and near-infrared study of the MGRO J2019+37 region
DOI: 10.1051/0004-6361/200912448 Bibcode: 2009A&A...507..241P

Luque-Escamilla, P. L.; Paredes, J. M.; Romero, G. E. +10 more

Context: MGRO J2019+37 is an unidentified extended source of very high energy gamma-rays originally reported by the Milagro Collaboration as the brightest TeV source in the Cygnus region. Its extended emission could be powered by either a single or several sources. The GeV pulsar AGL J2020.5+3653, discovered b…

2009 Astronomy and Astrophysics
XMM-Newton 21
2XMMiJ225036.9+573154 - a new eclipsing AMHer binary discovered using XMM-Newton
DOI: 10.1111/j.1365-2966.2009.14528.x Bibcode: 2009MNRAS.395..416R

Barclay, Thomas; Ramsay, Gavin; Hakala, Pasi +1 more

We report the discovery of an eclipsing polar, 2XMMiJ225036.9+573154, using XMM-Newton. It was discovered by searching the light curves in the 2XMMi catalogue for objects showing X-ray variability. Its X-ray light curve shows a total eclipse of the white dwarf by the secondary star every 174min. An extended pre-eclipse absorption dip is observed i…

2009 Monthly Notices of the Royal Astronomical Society
XMM-Newton 21
Saturn: Composition and Chemistry
DOI: 10.1007/978-1-4020-9217-6_5 Bibcode: 2009sfch.book...83F

Fouchet, Thierry; Moses, Julianne I.; Conrath, Barney J.

The chapter reviews our current knowledge of the molecular, elemental, and isotopic composition and atmospheric chemistry in Saturn 's shallow atmosphere, i.e., between the cloud levels and the homopause. We do not restrict the review to Cassini 's results, as past and current ground-based or Earth-based observations are still fundamental to draw …

2009 Saturn from Cassini-Huygens
Cassini 21
The coupling of winds, aerosols and chemistry in Titan's atmosphere
DOI: 10.1098/rsta.2008.0243 Bibcode: 2009RSPTA.367..665L

Lebonnois, Sebastien; Rannou, Pascal; Hourdin, Frederic

2009 Philosophical Transactions of the Royal Society of London Series A
Cassini 21