Search Publications

Cluster observations of simultaneous resonant interactions of ULF waves with energetic electrons and thermal ion species in the inner magnetosphere
DOI: 10.1029/2009JA014542 Bibcode: 2010JGRA..115.2214Y

Zong, Q. -G.; Reme, H.; Korth, A. +6 more

In this study, we report in situ observations on the simultaneous periodic modulations in the drifting energetic electrons (∼100 keV) and in the bouncing thermal ion species (O+ at ∼4.5 keV and H+ at ∼280 eV) with the same frequency of 3.3 mHz during the storm recovery phase on 21 October 2001. The Cluster fleet was traveling…

2010 Journal of Geophysical Research (Space Physics)
Cluster 54
X-QUEST: A Comprehensive X-ray Study of Local ULIRGS and QSOs
DOI: 10.1088/0004-637X/725/2/1848 Bibcode: 2010ApJ...725.1848T

Veilleux, Sylvain; Teng, Stacy H.

We present results from the X-ray portion of a multi-wavelength study of local ULIRGs and QSOs called QUEST (Quasar-ULIRG Evolution STudy). The data consist of new and archival X-ray data on 40 ULIRGs and 26 Palomar Green (PG) QSOs taken with Chandra and XMM-Newton. A combination of traditional and hardness ratio spectral fitting methods is used t…

2010 The Astrophysical Journal
XMM-Newton 54
Continued Cooling of the Crust in the Neutron Star Low-mass X-ray Binary KS 1731-260
DOI: 10.1088/2041-8205/722/2/L137 Bibcode: 2010ApJ...722L.137C

Miller, Jon M.; Cackett, Edward M.; Wijnands, Rudy +3 more

Some neutron star low-mass X-ray binaries have very long outbursts (lasting several years) which can generate a significant amount of heat in the neutron star crust. After the system has returned to quiescence, the crust then thermally relaxes. This provides a rare opportunity to study the thermal properties of neutron star crusts, putting constra…

2010 The Astrophysical Journal
XMM-Newton 54
The linear rms-flux relation in an ultraluminous X-ray source
DOI: 10.1111/j.1745-3933.2010.00864.x Bibcode: 2010MNRAS.405L..86H

Vaughan, S.; Heil, L. M.

We report the first detection of a linear correlation between rms variability amplitude and flux in the ultraluminous X-ray source (ULX) NGC 5408 X-1. The rms-flux relation has previously been observed in several galactic black hole X-ray binaries (BHBs), several active galactic nuclei (AGN) and at least one neutron star X-ray binary. This result …

2010 Monthly Notices of the Royal Astronomical Society
XMM-Newton 54
Cluster observations of bidirectional beams caused by electron trapping during antiparallel reconnection
DOI: 10.1029/2009JA014650 Bibcode: 2010JGRA..115.3214E

Fazakerley, A.; Egedal, J.; Lê, A. +4 more

So-called bidirectional electron beams have been observed by a number of spacecraft missions mainly in the inflow of reconnection regions. Here we show that these beam-like features in the electron distribution function are explained by electron trapping. The trapping is mainly controlled by a positive acceleration potential, Φ$\parallel$

2010 Journal of Geophysical Research (Space Physics)
Cluster 54
The number density of superdense early-type galaxies at 1 < z < 2 and the local cluster galaxies
DOI: 10.1111/j.1745-3933.2010.00920.x Bibcode: 2010MNRAS.408L..21S

Longhetti, M.; Gargiulo, A.; Saracco, P.

Many of the early-type galaxies (ETGs) observed so far at z > 1 turned out to have smaller radii with respect to that of a typical present day ETG with comparable mass. This has generated the conviction that in the past ETGs were more compact, hence denser, and that as a consequence, they should have increased their radius across the time to re…

2010 Monthly Notices of the Royal Astronomical Society
eHST 54
On the Progenitor and Supernova of the SN 2002cx-like Supernova 2008ge
DOI: 10.1088/0004-6256/140/5/1321 Bibcode: 2010AJ....140.1321F

Foley, Ryan J.; Rest, Armin; Phillips, Mark M. +6 more

We present observations of supernova (SN) 2008ge, which is spectroscopically similar to the peculiar SN 2002cx, and its pre-explosion site indicating that its progenitor was probably a white dwarf. NGC 1527, the host galaxy of SN 2008ge, is an S0 galaxy with no evidence of star formation or massive stars. Astrometrically matching late-time imaging…

2010 The Astronomical Journal
eHST 54
First results from HerMES on the evolution of the submillimetre luminosity function
DOI: 10.1051/0004-6361/201014675 Bibcode: 2010A&A...518L..23E

Altieri, B.; Aussel, H.; Elbaz, D. +81 more

We have carried out two extremely deep surveys with SPIRE, one of the two cameras on Herschel, at 250 µm, close to the peak of the far-infrared background. We have used the results to investigate the evolution of the rest-frame 250-µm luminosity function out to z = 2. We find evidence for strong evolution out to z ≃ 1 but evidence for …

2010 Astronomy and Astrophysics
Herschel 54
Thermo-dynamic and chemical properties of the intra-cluster medium
DOI: 10.1051/0004-6361/200913094 Bibcode: 2010A&A...510A..82L

Rossetti, M.; Molendi, S.; Leccardi, A.


Aims: We aim to provide constraints on evolutionary scenarios in clusters. One of our main goals is to understand whether, as claimed by some, the cool core/non-cool core division is established once and for all during the early history of a cluster.
Methods: We employ a sample of ≃60 objects to classify clusters according to different p…

2010 Astronomy and Astrophysics
XMM-Newton 54
The 2009 December Gamma-ray Flare of 3C 454.3: The Multifrequency Campaign
DOI: 10.1088/2041-8205/716/2/L170 Bibcode: 2010ApJ...716L.170P

Sakamoto, T.; Pian, E.; Fugazza, D. +81 more

During the month of 2009 December, the blazar 3C 454.3 became the brightest gamma-ray source in the sky, reaching a peak flux F ~ 2000 × 10-8 photons cm-2 s-1 for E > 100 MeV. Starting in 2009 November intensive multifrequency campaigns monitored the 3C 454 gamma-ray outburst. Here, we report on the results of a…

2010 The Astrophysical Journal
INTEGRAL 54