Search Publications

Flux transfer events simultaneously observed by Polar and Cluster: Flux rope in the subsolar region and flux tube addition to the polar cusp
DOI: 10.1029/2007JA012377 Bibcode: 2008JGRA..113.1205L

Russell, C. T.; RèMe, H.; Lucek, E. A. +9 more

In this paper we present observational evidence of a flux transfer event observed simultaneously at low-latitude by Polar and at high-latitude by Cluster. This event occurs on 21 March 2002, when both Cluster and Polar are located near local noon but with a large latitudinal separation. During the event, Cluster is moving outbound from the polar c…

2008 Journal of Geophysical Research (Space Physics)
Cluster 13
The Hubble Legacy Archive NICMOS grism data
DOI: 10.1051/0004-6361:200810282 Bibcode: 2008A&A...490.1165F

Kümmel, M.; Haase, J.; Kuntschner, H. +6 more

The Hubble Legacy Archive (HLA) aims to create calibrated science data from the Hubble Space Telescope archive and make them accessible via user-friendly and Virtual Observatory (VO) compatible interfaces. It is a collaboration between the Space Telescope Science Institute (STScI), the Canadian Astronomy Data Centre (CADC) and the Space Telescope …

2008 Astronomy and Astrophysics
eHST 13
The Planck cluster survey
DOI: 10.1002/asna.200710900 Bibcode: 2008AN....329..147B

Arnaud, M.; Bartlett, J. G.; Chamballu, A. +2 more

The Planck Satellite will survey the entire sky in 9 millimeter/submillimeter bands and detect thousands of galaxy clusters via their thermal Sunyaev-Zel'dovich (SZ) effect. The unprecedented volume of the survey will permit the construction of a unique catalog of massive clusters out to redshifts of order unity. We describe the expected contents …

2008 Astronomische Nachrichten
XMM-Newton 13
Bulk Compton motion in the luminous quasar 4C04.42?
DOI: 10.1111/j.1745-3933.2008.00498.x Bibcode: 2008MNRAS.388L..54D

de Rosa, A.; Ubertini, P.; Malizia, A. +2 more

We present the broadband analysis of the powerful quasar 4C04.42 (z = 0.965) observed by XMM-Newton and INTEGRAL. The 0.2-200keV spectrum is well reproduced with a hard power-law component (Γ ~ 1.2), augmented by a soft component below 2keV (observer frame), which is described by a thermal blackbody with temperature kT ⋍ 0.15keV. Alternatively, a …

2008 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 13
Sequestration of Noble Gases by H+3 in Protoplanetary Disks and Outer Solar System Composition
DOI: 10.1086/523925 Bibcode: 2008ApJ...673..637M

Ceccarelli, C.; Mousis, O.; Pauzat, F. +1 more

We study the efficiency of the noble gas sequestration by the ion H+3 in the form of X H+3 complexes (with X = argon , krypton, or xenon) in gas-phase conditions similar to those encountered during the cooling of protoplanetary disks. We show that X H+3 complexes form very stable st…

2008 The Astrophysical Journal
Huygens 13
XMM-Newton studies of a massive cluster of galaxies: RXC J2228.6+2036
DOI: 10.1051/0004-6361:200809699 Bibcode: 2008A&A...489....1J

Böhringer, H.; Pointecouteau, E.; Chen, Y. +2 more

We present the X-ray properties of a massive cluster of galaxies (RXC J2228.6+2036 at z = 0.421) using XMM-Newton data. The X-ray mass modeling is based on the temperature and density distributions of the intracluster medium derived using a deprojection method. We find that RXC J2228.6+2036 is a hot cluster (T500=8.92^+1.78-1.32

2008 Astronomy and Astrophysics
XMM-Newton 13
Evidence for Resonance Line Scattering in the Suzaku X-Ray Spectrum of the Cygnus Loop
DOI: 10.1093/pasj/60.3.521 Bibcode: 2008PASJ...60..521M

Hughes, John P.; Miyata, Emi; Masai, Kuniaki

We present an analysis of the Suzaku observation of the northeastern rim of the Cygnus Loop supernova remnant. The high detection efficiency together with the high spectral resolution of the Suzaku X-ray CCD camera enables us to detect highly-ionized C and N emission lines from the Cygnus Loop. Given the significant plasma structure within the Suz…

2008 Publications of the Astronomical Society of Japan
Suzaku 13
Source Matching in the SDSS and Rass: which Galaxies are Really X-Ray Sources?
DOI: 10.1088/0004-6256/135/1/10 Bibcode: 2008AJ....135...10P

Hoyle, Fiona; Parejko, John K.; Constantin, Anca +1 more

The current view of galaxy formation holds that all massive galaxies harbor a massive black hole at their center, but that these black holes are not always in an actively accreting phase. X-ray emission is often used to identify accreting sources, but for galaxies that are not harboring quasars (low-luminosity active galaxies), the X-ray flux may …

2008 The Astronomical Journal
XMM-Newton 13
The Nearby and Extremely Metal-poor Galaxy CGCG 269-049
DOI: 10.1086/524399 Bibcode: 2008ApJ...675..194C

Windhorst, Rogier A.; Kim, Hwihyun; Jansen, Rolf A. +2 more

We present Hubble Space Telescope (HST) and Spitzer Space Telescope images and photometry of the extremely metal-poor (Zcong 0.03 Z) blue dwarf galaxy CGCG 269-049. The HST images reveal a large population of red giant and asymptotic giant branch stars, ruling out the possibility that the galaxy has recently formed. From the magnitude …

2008 The Astrophysical Journal
eHST 13
On the relation between DC current locations and an EUV bright point: A case study
DOI: 10.1051/0004-6361:200809975 Bibcode: 2008A&A...490..345S

Madjarska, M. S.; Büchner, J.; Santos, J. C. +1 more

Context: Motion of the photospheric plasma forces the footpoints of magnetic flux tubes to move. This can give rise to electric currents in the solar atmosphere. The dissipation of these electric currents and the consequent heating of the solar plasma may be responsible for the formation of Extreme-UltraViolet (EUV) and X-ray bright points. Earlie…

2008 Astronomy and Astrophysics
SOHO 13