Search Publications

Quintessential inflation with canonical and noncanonical scalar fields and Planck 2015 results
DOI: 10.1103/PhysRevD.92.023522 Bibcode: 2015PhRvD..92b3522G

Geng, Chao-Qiang; Saridakis, Emmanuel N.; Myrzakulov, R. +2 more

We investigate two classes of models of quintessential inflation, based upon canonical as well as noncanonical scalar fields. In particular, introducing potentials steeper than the standard exponential, we construct models that can give rise to a successful inflationary phase, with signatures consistent with Planck 2015 results. Additionally, usin…

2015 Physical Review D
Planck 94
The Complex Accretion Geometry of GX 339-4 as Seen by NuSTAR and Swift
DOI: 10.1088/0004-637X/808/2/122 Bibcode: 2015ApJ...808..122F

Harrison, F. A.; Stern, D.; Zhang, W. W. +19 more

We present spectral analyses of five Nuclear Spectroscopic Telescope Array and Swift observations of GX 339-4 taken during a failed outburst during the summer of 2013. These observations cover Eddington luminosity fractions in the range ≈0.9%-6%. Throughout this outburst GX 339-4 stayed in the hard state and all five observations show similar X-ra…

2015 The Astrophysical Journal
XMM-Newton 94
The Martian atmospheric ion escape rate dependence on solar wind and solar EUV conditions: 1. Seven years of Mars Express observations
DOI: 10.1002/2015JE004816 Bibcode: 2015JGRE..120.1298R

Barabash, Stas; Nilsson, Hans; Holmström, Mats +3 more

More than 7 years of ion flux measurements in the energy range 10 eV-15 keV have allowed the ASPERA-3/IMA (Analyzer of Space Plasmas and Energetic Ions/Ion Mass Analyzer) instrument on Mars Express to collect a large database of ion measurements in the Mars environment, over a wide range of upstream solar wind (density and velocity) and radiation …

2015 Journal of Geophysical Research (Planets)
MEx 93
X-Ray and Radio Emission from Type IIn Supernova SN 2010jl
DOI: 10.1088/0004-637X/810/1/32 Bibcode: 2015ApJ...810...32C

Chandra, Poonam; Fransson, Claes; Chevalier, Roger A. +2 more

We present all X-ray and radio observations of the Type IIn supernova SN 2010jl. The X-ray observations cover a period up to day 1500 with Chandra, XMM-Newton, NuSTAR, and Swift-X-ray Telescope (XRT). The Chandra observations after 2012 June, the XMM-Newton observation in 2013 November, and most of the Swift-XRT observations until 2014 December ar…

2015 The Astrophysical Journal
XMM-Newton 93
The Formation of IRIS Diagnostics. IV. The Mg II Triplet Lines as a New Diagnostic for Lower Chromospheric Heating
DOI: 10.1088/0004-637X/806/1/14 Bibcode: 2015ApJ...806...14P

De Pontieu, Bart; Hansteen, Viggo; Carlsson, Mats +1 more

A triplet of subordinate lines of Mg ii exists in the region around the h&k lines. In solar spectra these lines are seen mostly in absorption, but in some cases can become emission lines. The aim of this work is to study the formation of this triplet, and investigate any diagnostic value they can bring. Using 3D radiative magnetohydrodynamic s…

2015 The Astrophysical Journal
IRIS 93
CHAOS II. Gas-phase Abundances in NGC 5194
DOI: 10.1088/0004-637X/808/1/42 Bibcode: 2015ApJ...808...42C

Skillman, Evan D.; Moustakas, John; Croxall, Kevin V. +2 more

We have observed NGC 5194 (M51a) as part of the CHemical Abundances of Spirals project. Using the Multi Object Double Spectrographs on the Large Binocular Telescope we are able to measure one or more of the temperature-sensitive auroral lines ([O iii] λ4363, [N ii] λ5755, [S iii] λ6312) and thus measure “direct” gas-phase abundances in 29 individu…

2015 The Astrophysical Journal
eHST 93
Diversity in extinction laws of Type Ia supernovae measured between 0.2 and 2 µm
DOI: 10.1093/mnras/stv1505 Bibcode: 2015MNRAS.453.3300A

Dahle, H.; Lundqvist, P.; Östlin, G. +36 more

We present ultraviolet (UV) observations of six nearby Type Ia supernovae (SNe Ia) obtained with the Hubble Space Telescope, three of which were also observed in the near-IR (NIR) with Wide-Field Camera 3. UV observations with the Swift satellite, as well as ground-based optical and NIR data provide complementary information. The combined data set…

2015 Monthly Notices of the Royal Astronomical Society
eHST 93
Possible binary progenitors for the Type Ib supernova iPTF13bvn
DOI: 10.1093/mnras/stu2197 Bibcode: 2015MNRAS.446.2689E

Fraser, Morgan; Eldridge, J. J.; Smartt, Stephen J. +1 more

Cao et al. reported a possible progenitor detection for the Type Ib supernovae iPTF13bvn for the first time. We find that the progenitor is in fact brighter than the magnitudes previously reported by approximately 0.7-0.2 mag with a larger error in the bluer filters. We compare our new magnitudes to our large set of binary evolution models and fin…

2015 Monthly Notices of the Royal Astronomical Society
eHST 93
Asteroseismic inference on rotation, gyrochronology and planetary system dynamics of 16 Cygni
DOI: 10.1093/mnras/stu2331 Bibcode: 2015MNRAS.446.2959D

García, R. A.; Chaplin, W. J.; Lund, M. N. +13 more

The solar analogues 16 Cyg A and B are excellent asteroseismic targets in the Kepler field of view and together with a red dwarf and a Jovian planet form an interesting system. For these more evolved Sun-like stars we cannot detect surface rotation with the current Kepler data but instead use the technique of asteroseimology to determine rotationa…

2015 Monthly Notices of the Royal Astronomical Society
SOHO 92
Molecular gas content in strongly lensed z ~ 1.5-3 star-forming galaxies with low infrared luminosities
DOI: 10.1051/0004-6361/201424661 Bibcode: 2015A&A...577A..50D

Kneib, J. -P.; Schaerer, D.; Dessauges-Zavadsky, M. +10 more

To extend the molecular gas measurements to more typical star-forming galaxies (SFGs) with star formation rates SFR< 40 M yr-1 and stellar masses M< 2.5 × 1010M at z ~ 1.5-3, we have observed CO emission with the IRAM Plateau de Bure Interferometer and the IRAM 30 m telescope for five…

2015 Astronomy and Astrophysics
Herschel 92