Search Publications

Post-Planck dark energy constraints
DOI: 10.1103/PhysRevD.91.083005 Bibcode: 2015PhRvD..91h3005H

Hazra, Dhiraj Kumar; Pal, Supratik; Sen, Anjan A. +2 more

We constrain plausible dark energy models using the recently published cosmic microwave background (CMB) temperature anisotropy data from Planck together with WMAP9 low-ℓ polarization data and the data from low redshift surveys. To circumvent the limitations of any particular equation of state toward describing all existing dark energy models, we …

2015 Physical Review D
Planck 34
Total electron content in the Martian atmosphere: A critical assessment of the Mars Express MARSIS data sets
DOI: 10.1002/2014JA020630 Bibcode: 2015JGRA..120.2166S

Gurnett, D. A.; Lester, M.; Morgan, D. D. +14 more

The total electron content (TEC) is one of the most useful parameters to evaluate the behavior of the Martian ionosphere because it contains information on the total amount of free electrons, the main component of the Martian ionospheric plasma. The Mars Express Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) radar is able to d…

2015 Journal of Geophysical Research (Space Physics)
MEx 33
Charge exchange in cometary coma: Discovery of H- ions in the solar wind close to comet 67P/Churyumov-Gerasimenko
DOI: 10.1002/2015GL064504 Bibcode: 2015GeoRL..42.5125B

Goldstein, R.; Mokashi, P.; Tzou, C. -Y. +4 more

As Rosetta was orbiting comet 67P/Churyumov-Gerasimenko, the Ion and Electron Sensor detected negative particles with angular distributions like those of the concurrently measured solar wind protons but with fluxes of only about 10% of the proton fluxes and energies of about 90% of the proton energies. Using well-known cross sections and energy-lo…

2015 Geophysical Research Letters
Rosetta 33
Multi-spacecraft Measurement of Turbulence within a Magnetic Reconnection Jet
DOI: 10.1088/2041-8205/815/2/L24 Bibcode: 2015ApJ...815L..24O

Khotyaintsev, Yu. V.; Matthaeus, W. H.; Chapman, S. C. +3 more

The relationship between magnetic reconnection and plasma turbulence is investigated using multipoint in situ measurements from the Cluster spacecraft within a high-speed reconnection jet in the terrestrial magnetotail. We show explicitly that work done by electromagnetic fields on the particles, {\boldsymbol{J}}\cdot {\boldsymbol{E}}, has a non-G…

2015 The Astrophysical Journal
Cluster 33
Star-formation histories of local luminous infrared galaxies
DOI: 10.1051/0004-6361/201425359 Bibcode: 2015A&A...577A..78P

Pérez-González, Pablo G.; Arribas, Santiago; Colina, Luis +7 more

We present analysis of the integrated spectral energy distribution (SED) from the ultraviolet (UV) to the far-infrared and Hα of a sample of 29 local systems and individual galaxies with infrared (IR) luminosities between 1011L and 1011.8L. We combined new narrow-band Hα + [N ii] and broad-band g, r op…

2015 Astronomy and Astrophysics
Herschel 33
Hydrogen Ly-α and Ly-β full Sun line profiles observed with SUMER/SOHO (1996-2009)
DOI: 10.1051/0004-6361/201526059 Bibcode: 2015A&A...581A..26L

Vial, J. -C.; Wilhelm, K.; Curdt, W. +2 more

Context. Accurate hydrogen spectra emitted by the entire solar disc in the Ly-α and Ly-βlines are valuable for deriving the distribution and the behaviour of atomic hydrogen in the heliosphere, for understanding the UV emissions of solar type stars better, and finally for estimating the solar energy input that mainly initiates the chemical process…

2015 Astronomy and Astrophysics
SOHO 33
Interplay between heartbeat oscillations and wind outflow in microquasar IGR J17091-3624
DOI: 10.1051/0004-6361/201425003 Bibcode: 2015A&A...574A..92J

Bianchi, Stefano; Janiuk, Agnieszka; Capitanio, Fiamma +1 more


Aims: During the bright outburst in 2011, the black hole candidate IGR J17091-3624 exhibited strong quasi-periodic flare-like events (on timescales of tens of seconds) in some characteristic states, the so-called heartbeat state. From the theoretical point of view, these oscillations may be modeled by the process of accretion disk instability…

2015 Astronomy and Astrophysics
INTEGRAL XMM-Newton 33
Infrared emission of young HII regions: a Herschel/Hi-GAL study
DOI: 10.1051/0004-6361/201525953 Bibcode: 2015A&A...579A..71C

Smith, M. D.; Testi, L.; Molinari, S. +7 more

Context. Investigating the relationship between radio and infrared emission of Hii regions may help shed light on the nature of the ionizing stars and the formation mechanism of early-type stars in general.
Aims: We have taken advantage of recent unbiased surveys of the Galactic plane such as Herschel/Hi-GAL and VLA/CORNISH to study a bona fi…

2015 Astronomy and Astrophysics
Herschel 33
Evidence for High-frequency QPOs with a 3:2 Frequency Ratio from a 5000 Solar Mass Black Hole
DOI: 10.1088/2041-8205/811/1/L11 Bibcode: 2015ApJ...811L..11P

Cenko, S. Bradley; Zoghbi, Abderahmen; Tombesi, Francesco +3 more

Following the discovery of 3:2 resonance quasi-periodic oscillations (QPOs) in M82X-1, we have constructed power density spectra (PDS) of all 15 (sufficiently long) XMM-Newton observations of the ultraluminous X-ray source NGC 1313 X-1 (LX ≈ 2 × 1040 erg s-1). We detect a strong QPO at a frequency of 0.29 ± 0.01 Hz…

2015 The Astrophysical Journal
XMM-Newton 33
Gale crater and impact processes - Curiosity's first 364 Sols on Mars
DOI: 10.1016/j.icarus.2014.10.013 Bibcode: 2015Icar..249..108N

Bridges, Nathan T.; Mangold, Nicolas; Wiens, Roger C. +18 more

Impact processes at all scales have been involved in the formation and subsequent evolution of Gale crater. Small impact craters in the vicinity of the Curiosity MSL landing site and rover traverse during the 364 Sols after landing have been studied both from orbit and the surface. Evidence for the effect of impacts on basement outcrops may includ…

2015 Icarus
MEx 33