Search Publications

Characterizing the Radio-X-ray Connection in GRS 1915+105
DOI: 10.1088/0004-637X/717/2/1222 Bibcode: 2010ApJ...717.1222P

Rodriguez, J.; Pooley, G. G.; Prat, L.

We analyzed radio and X-ray observations of GRS 1915+105, between 1995 May and 2006 June, focusing on the times characterized by radio flares and cycles of hard dips—soft spikes in the X-ray light curve. Assuming these flares to be discrete ejections, we applied a plasmon model to the radio data, with good agreement with the light curves. We fitte…

2010 The Astrophysical Journal
INTEGRAL 13
The far-ultraviolet albedo of Šteins measured with Rosetta-ALICE
DOI: 10.1016/j.pss.2010.03.005 Bibcode: 2010P&SS...58.1088A

Parker, Joel Wm.; Bertaux, Jean-Loup; Weaver, Harold A. +9 more

During Rosetta's flyby of the asteroid (2867) Šteins in 2008, we used the ALICE instrument to measure the first far-ultraviolet (FUV) reflectivity spectrum of an asteroid (850-2000 Å). It is very dark in the FUV, ∼4%, compared to its very high reflectivity (40%) at optical wavelengths. The FUV albedo does not exhibit a systematic color trend acros…

2010 Planetary and Space Science
Rosetta 13
On the relationship between coronal heating, magnetic flux, and the density of the solar wind
DOI: 10.1029/2009JA015131 Bibcode: 2010JGRA..115.6104R

McComas, D. J.; Schwadron, N. A.; Riley, Pete +3 more

The stark differences between the current solar minimum and the previous one offer a unique opportunity to develop new constraints on mechanisms for heating and acceleration of the solar wind. We have used a combination of numerical simulations and analysis of remote solar and in situ observations to infer that the coronal heating rate, H, scales …

2010 Journal of Geophysical Research (Space Physics)
Ulysses 13
Impact of Coherent Backscattering on the Spectra of Icy Satellites of Saturn and the Implications of Its Effects for Remote Sensing
DOI: 10.1088/2041-8205/711/2/L71 Bibcode: 2010ApJ...711L..71K

Buratti, B.; Kolokolova, L.; Tishkovets, V.

We have found systematic variations in the spectra of Saturn's icy satellites Rhea and Iapetus obtained by the Cassini Visual and Infrared Mapping Spectrometer (VIMS). The main attribute of these variations is a significantly different depth of the absorption bands at different phase angles. We show that these variations likely result from the coh…

2010 The Astrophysical Journal
Cassini 13
A Limit on the Number of Isolated Neutron Stars Detected in the ROSAT All-Sky-Survey Bright Source Catalog
DOI: 10.1088/0004-637X/714/2/1424 Bibcode: 2010ApJ...714.1424T

Fox, Derek B.; Rutledge, Robert E.; Turner, Monica L. +2 more

Using new and archival observations made with the Swift satellite and other facilities, we examine 147 X-ray sources selected from the ROSAT All-Sky-Survey Bright Source Catalog (RASS/BSC) to produce a new limit on the number of isolated neutron stars (INSs) in the RASS/BSC, the most constraining such limit to date. Independent of X-ray spectrum a…

2010 The Astrophysical Journal
XMM-Newton 13
Measurements of stray antenna capacitance in the STEREO/WAVES instrument: Comparison of the measured voltage spectrum with an antenna electron shot noise model
DOI: 10.1029/2009RS004194 Bibcode: 2010RaSc...45.1005Z

Eastwood, J. P.; Maksimovic, M.; Bale, S. D. +6 more

One of the most accurate techniques for in situ measuring the electron density and temperature in space plasmas is the quasi-thermal noise spectroscopy, which uses the voltage fluctuation spectrum on an electric antenna. This technique has been used successfully on the WIND and ULYSSES spacecraft; however, on STEREO this technique may only work in…

2010 Radio Science
Ulysses 13
Aerosols in Titan's Atmosphere
DOI: 10.1007/978-1-4020-9215-2_12 Bibcode: 2010tfch.book..297T

West, Robert A.; Tomasko, Martin G.

Aerosols in Titan's atmosphere play important roles in the transfer of solar and thermal radiation, in Titan's heat balance, in forcing atmospheric dynamics, and as a sink for photochemical reactions. In this chapter we briefly summarize the history of our knowledge of their distribution and optical properties before concentrating in greater detai…

2010 Titan from Cassini-Huygens
Cassini 13
Anti-correlated Soft Lags in the Intermediate State of Black Hole Source GX 339-4
DOI: 10.1088/0004-637X/725/1/1317 Bibcode: 2010ApJ...725.1317S

Rao, A. R.; Sriram, K.; Choi, C. S.

We report the few hundred second anti-correlated soft lags between soft and hard energy bands in the source GX 339-4 using RXTE observations. In one observation, anti-correlated soft lags were observed using the ISGRI/INTEGRAL hard energy band and the PCA/RXTE soft energy band light curves. The lags were observed when the source was in hard and so…

2010 The Astrophysical Journal
INTEGRAL 13
The non-evolving internal structure of early-type galaxies: the case study SDSSJ0728+3835 at z = 0.206
DOI: 10.1111/j.1365-2966.2010.16881.x Bibcode: 2010MNRAS.406.2339B

Treu, Tommaso; Gavazzi, Raphaël; Auger, Matthew W. +4 more

We study the internal dynamical structure of the early-type lens galaxy SDSSJ0728+3835 at z = 0.206. The analysis is based on two-dimensional kinematic maps extending out to 1.7 effective radii obtained from Keck spectroscopy, on lensing geometry and on stellar mass estimates obtained from multiband Hubble Space Telescope imaging. The data are mod…

2010 Monthly Notices of the Royal Astronomical Society
eHST 13
XMM-Newton long-look observation of the narrow line Seyfert 1 galaxy PKS 0558-504. I. Spectral analysis
DOI: 10.1051/0004-6361/200913289 Bibcode: 2010A&A...510A..65P

Papadakis, I. E.; Brinkmann, W.; Nicastro, F. +3 more

Context. PKS 0558-504 has been observed repeatedly by XMM-Newton as a calibration and performance verification (PV) target. In this work, we present results from the spectral analysis of a long XMM-Newton observation of the radio loud Narrow Line Seyfert 1 galaxy PKS 0558-504.
Aims: To study the soft excess component in this object, the spect…

2010 Astronomy and Astrophysics
XMM-Newton 13