Search Publications

Cosmological constraints from the observed angular cross-power spectrum between Sunyaev-Zel'dovich and X-ray surveys
DOI: 10.1051/0004-6361/201425555 Bibcode: 2015A&A...576A..90H

Aghanim, N.; Diego, J. M.; Douspis, M. +3 more

We present the first detection of the cross-correlation angular power spectrum between the thermal Sunyaev-Zel'dovich (tSZ) effect and the X-ray emission over the full sky. The tSZ effect and X-rays are produced by the same hot gas within groups and clusters of galaxies, which creates a naturally strong correlation between them that can be used to…

2015 Astronomy and Astrophysics
Planck 22
Linking Europa's plume activity to tides, tectonics, and liquid water
DOI: 10.1016/j.icarus.2015.02.023 Bibcode: 2015Icar..253..169R

Roth, Lorenz; Rhoden, Alyssa Rose; Retherford, Kurt +1 more

Much of the geologic activity preserved on Europa's icy surface has been attributed to tidal deformation, mainly due to Europa's eccentric orbit. Although the surface is geologically young (30-80 Myr), there is little information as to whether tidally-driven surface processes are ongoing. However, a recent detection of water vapor near Europa's so…

2015 Icarus
eHST 22
UV Insights into the Complex Populations of M87 Globular Clusters
DOI: 10.1088/0004-637X/805/2/178 Bibcode: 2015ApJ...805..178B

Anderson, J.; Milone, A. P.; Bedin, L. R. +7 more

We have imaged with Hubble Space Telescope WFC3/UVIS the central 2\buildrel{ \prime}\over{.} 7× 2\buildrel{ \prime}\over{.} 7 region of the giant elliptical galaxy M87, using the ultraviolet filter F275W. In combination with archival ACS/WFC data taken through the F606W and F814W filters, covering the same field, we have constructed integrated-lig…

2015 The Astrophysical Journal
eHST 22
XMM-Newton large program on SN1006 - I. Methods and initial results of spatially resolved spectroscopy
DOI: 10.1093/mnras/stv1882 Bibcode: 2015MNRAS.453.3953L

Vink, Jacco; Miceli, Marco; Bocchino, Fabrizio +2 more

Based on our newly developed methods and the XMM-Newton large program of SN1006, we extract and analyse the spectra from 3596 tessellated regions of this supernova remnant (SNR) each with 0.3-8 keV counts >104. For the first time, we map out multiple physical parameters, such as the temperature (kT), electron density (ne),…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 22
Far-Infrared and Accretion Luminosities of the Present-day Active Galactic Nuclei
DOI: 10.1088/0004-637X/807/1/28 Bibcode: 2015ApJ...807...28M

Woo, Jong-Hak; Matsuoka, Kenta

We investigate the relation between star formation (SF) and black hole accretion luminosities, using a sample of 492 type-2 active galactic nuclei (AGNs) at z\lt 0.22, which are detected in the far-infrared (FIR) surveys with AKARI and Herschel. We adopt FIR luminosities at 90 and 100 µm as SF luminosities, assuming the proposed linear propo…

2015 The Astrophysical Journal
AKARI Herschel 22
Understanding the Internal Chemical Composition and Physical Processes of the Solar Interior
DOI: 10.1007/s11214-014-0035-9 Bibcode: 2015SSRv..196...49B

Basu, Sarbani; Turck-Chièze, Sylvaine; Grevesse, Nicolas +1 more

The Sun, the closest and most well studied of stars, is generally used as a standard that other stars are compared to. Models of the Sun are constantly tested with helioseismic data. These data allow us to probe the internal structure and dynamics of the Sun. Among the main sources of the data is the SOHO spacecraft that has been continuously obse…

2015 Space Science Reviews
SOHO 22
Direction of interstellar hydrogen flow in the heliosphere: theoretical modelling and comparison with SOHO/SWAN data
DOI: 10.1093/mnras/stu2218 Bibcode: 2015MNRAS.446.2929K

Katushkina, O. A.; Izmodenov, V. V.; Alexashov, D. B.

The analysis of SOlar and Heliospheric Observatory (SOHO) Solar Wind ANisotropies (SWAN) data for backscattered solar Lyman α radiation performed by Lallement et al. showed for the first time that the average direction of interstellar hydrogen flow in the heliosphere is deflected by several degrees relative to the original direction of the interst…

2015 Monthly Notices of the Royal Astronomical Society
SOHO 22
Far-UV Spectroscopy of the Planet-hosting Star WASP-13: High-energy Irradiance, Distance, Age, Planetary Mass-loss Rate, and Circumstellar Environment
DOI: 10.1088/0004-637X/815/2/118 Bibcode: 2015ApJ...815..118F

France, K.; Fossati, L.; Lendl, M. +3 more

Several transiting hot Jupiters orbit relatively inactive main-sequence stars. For some of those, the {log}{R}{HK}\prime activity parameter lies below the basal level (-5.1). Two explanations have been proposed so far: (i) the planet affects the stellar dynamo, (ii) the {log}{R}{HK}\prime measurements …

2015 The Astrophysical Journal
eHST 22
Observational hints of a pre-inflationary scale?
DOI: 10.1142/S0218271815440083 Bibcode: 2015IJMPD..2444008G

Gruppuso, A.; Sagnotti, A.

We argue that the lack of power exhibited by cosmic microwave background (CMB) anisotropies at large angular scales might be linked to the onset of inflation. We highlight observational features and theoretical hints that support this view, and present a preliminary estimate of the physical scale that would underlie the phenomenon.

2015 International Journal of Modern Physics D
Planck 22
The eccentric short-period orbit of the supergiant fast X-ray transient HD 74194 (=LM Vel)
DOI: 10.1051/0004-6361/201527140 Bibcode: 2015A&A...583L...4G

Gamen, R.; Maíz Apellániz, J.; Alfaro, E. J. +5 more

Aims. We present the first orbital solution for the O-type supergiant star HD 74194, which is the optical counterpart of the supergiant fast X-ray transient IGR J08408-4503. Methods. We measured the radial velocities in the optical spectrum of HD 74194, and we determined the orbital solution for the first time. We also analysed the complex Hα prof…

2015 Astronomy and Astrophysics
INTEGRAL 22