Search Publications

Properties of dust in the high-latitude translucent cloud L1780. I. Spatially distinct dust populations and increased dust emissivity from ISO observations
DOI: 10.1051/0004-6361:20053467 Bibcode: 2006A&A...451..961R

Juvela, M.; Lemke, D.; Lehtinen, K. +2 more

We have analyzed the properties of dust in the high galactic latitude translucent cloud Lynds 1780 using ISOPHOT maps at 100 µm and 200 µm and raster scans at 60 µm, 80 µm, 100 µm, 120 µm, 150 µm and 200 µm. In far-infrared (FIR) emission, the cloud has a single core that coincides with the maxima of…

2006 Astronomy and Astrophysics
ISO 34
X-ray continuum properties of GRB afterglows observed by XMM-Newton and Chandra
DOI: 10.1051/0004-6361:20053903 Bibcode: 2006A&A...455..803G

Piro, L.; Corsi, A.; Gendre, B.

We present a catalog of XMM-Newton and Chandra observations of gamma-ray burst (GRB) afterglows, reduced in a common way using the most up-to-date calibration files and software. We focus on the continuum properties of the afterglows. We derive the spectral and temporal decay indices for 16 bursts. We place constraints on the burst environment and…

2006 Astronomy and Astrophysics
XMM-Newton 34
On the compact nature of the most luminous ULX in the Cartwheel ring
DOI: 10.1111/j.1365-2966.2006.11116.x Bibcode: 2006MNRAS.373.1627W

Trinchieri, Ginevra; Wolter, Anna; Colpi, Monica

We report the first detection of flux variability in the most luminous X-ray source in the southern ring of the Cartwheel galaxy. XMM-Newton data show that the luminosity has varied over a time-scale of 6 months from L0.5-10keV ~ 1.3 × 1041ergs-1, consistent with the previous Chandra observation, to L0.5-10keV…

2006 Monthly Notices of the Royal Astronomical Society
XMM-Newton 34
The potential for prebiotic chemistry in the possible cryovolcanic dome Ganesa Macula on Titan
DOI: 10.1017/S1473550406002898 Bibcode: 2006IJAsB...5...57N

Lorenz, R. D.; Neish, C. D.; O'Brien, D. P. +1 more

New observations of Titan by the Cassini spacecraft suggest the presence of cryovolcanism on the surface. Cryovolcanism has important astrobiological implications, as it provides a means of exposing Titan's organics to liquid water, transforming hydrocarbons and nitriles into more evolved and oxidized prebiotic species. One possible cryovolcano - …

2006 International Journal of Astrobiology
Cassini 34
Simulations of thermally broadened H I Ly α absorption arising in the warm-hot intergalactic medium
DOI: 10.1051/0004-6361:20054556 Bibcode: 2006A&A...451..767R

Richter, P.; Fang, T.; Bryan, G. L.

Recent far-ultraviolet (FUV) absorption line measurements of low-redshift quasars have unveiled a population of intervening broad H i Ly α absorbers (BLAs) with large Doppler parameters (b≥ 40 km s-1). If the large width of these lines is dominated by thermal line broadening, the BLAs may trace highly-ionized gas in the warm-hot interga…

2006 Astronomy and Astrophysics
eHST 34
A Time-dependent Leptonic Model for Microquasar Jets: Application to LS I +61 303
DOI: 10.1086/508880 Bibcode: 2006ApJ...650L.123G

Gupta, S.; Böttcher, M.

The Galactic high-mass X-ray binary and jet source (microquasar) LS I +61 303 has recently been detected at TeV γ-ray energies by the MAGIC telescope. We have applied a time-dependent leptonic jet model to the broadband spectral energy distribution (SED), and we have suggested (although not unambiguously detected) an orbital modulation of the very…

2006 The Astrophysical Journal
INTEGRAL 34
Ultraviolet-bright, High-Redshift Ultraluminous Infrared Galaxies
DOI: 10.1086/500647 Bibcode: 2006ApJ...637L..89C

Woodgate, Bruce; Teplitz, Harry; Williger, Gerard M. +3 more

We present Spitzer Space Telescope observations of the z=2.38 Lyα emitter overdensity associated with galaxy cluster J2143-4423, the largest known structure (110 Mpc) above z=2. We imaged 22 of the 37 known Lyα emitters within the filament-like structure, using the MIPS 24 µm band. We detected six of the Lyα emitters, including three of the …

2006 The Astrophysical Journal
eHST 34
The Latitudinal Excursion of Coronal Magnetic Field Lines in Response to Differential Rotation: MHD Simulations
DOI: 10.1086/504289 Bibcode: 2006ApJ...642L..69L

Riley, Pete; Linker, Jon A.; Mikić, Zoran +1 more

Solar energetic particles, which are believed to originate from corotating interacting regions (CIRs) at low heliographic latitude, were observed by the Ulysses spacecraft even as it passed over the Sun's poles. One interpretation of this result is that high-latitude field lines intercepted by Ulysses connect to low-latitude CIRs at much larger he…

2006 The Astrophysical Journal
Ulysses 34
Solar Convection Zone Dynamics: How Sensitive Are Inversions to Subtle Dynamo Features?
DOI: 10.1086/506931 Bibcode: 2006ApJ...649.1155H

Thompson, M. J.; Howe, R.; Komm, R. +5 more

The nearly 10 year span of medium-degree helioseismic data from the Global Oscillation Network Group and the Michelson Doppler Imager has allowed us to study the evolving flows in the solar convection zone over most of solar cycle 23. Using two independent two-dimensional rotation inversion techniques and extensive studies of the resolution using …

2006 The Astrophysical Journal
SOHO 33
Light Curves of 20-100 km Kuiper Belt Objects Using the Hubble Space Telescope
DOI: 10.1086/499228 Bibcode: 2006AJ....131.1149T

Bernstein, Gary M.; Trilling, David E.

We report high-precision photometry of three small and one larger Kuiper Belt objects (KBOs) obtained with the Advanced Camera for Surveys on board the Hubble Space Telescope. The three small bodies are the smallest KBOs for which light-curve measurements are available. The object 2003 BF91 has a diameter of 20 km (assuming 10% albedo) …

2006 The Astronomical Journal
eHST 33