Search Publications

Broad absorption features in wind-dominated ultraluminous X-ray sources?
DOI: 10.1093/mnrasl/slt157 Bibcode: 2014MNRAS.438L..51M

Middleton, Matthew J.; Roberts, Timothy P.; Walton, Dominic J. +1 more

The luminosities of ultraluminous X-ray sources (ULXs) require an exotic solution with either supercritical accretion modes on to stellar-mass black holes or subcritical accretion on to intermediate-mass black holes (IMBHs) being invoked. Discriminating between the two is non-trivial due to the present lack of a direct mass measurement. A key expe…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 94
Azimuthally resolved X-ray spectroscopy to the edge of the Perseus Cluster
DOI: 10.1093/mnras/stt2209 Bibcode: 2014MNRAS.437.3939U

Simionescu, A.; Fabian, A. C.; Allen, S. W. +9 more

We present the results from extensive, new observations of the Perseus Cluster of galaxies, obtained as a Suzaku Key Project. The 85 pointings analysed span eight azimuthal directions out to 2° = 2.6 Mpc, to and beyond the virial radius r200 ∼ 1.8 Mpc, offering the most detailed X-ray measurements of the intracluster medium (ICM) at lar…

2014 Monthly Notices of the Royal Astronomical Society
Planck Suzaku 94
Deflected propagation of a coronal mass ejection from the corona to interplanetary space
DOI: 10.1002/2013JA019537 Bibcode: 2014JGRA..119.5117W

Wang, Yuming; Shen, Fang; Shen, Chenglong +2 more

Among various factors affecting the space weather effects of a coronal mass ejection (CME), its propagation trajectory in the interplanetary space is an important one determining whether and when the CME will hit the Earth. Many direct observations have revealed that a CME may not propagate along a straight trajectory in the corona, but whether or…

2014 Journal of Geophysical Research (Space Physics)
SOHO 94
Wiggly whipped inflation
DOI: 10.1088/1475-7516/2014/08/048 Bibcode: 2014JCAP...08..048H

Starobinsky, Alexei A.; Hazra, Dhiraj Kumar; Smoot, George F. +1 more

Motivated by BICEP2 results on the CMB polarization B-mode which imply primordial gravitational waves are produced when the Universe has the expansion rate of about H ≈ 1014 GeV, and by deviations from a smooth power-law behavior for multipoles ℓ <50 in the CMB temperature anisotropy power spectrum found in the WMAP and Planck experi…

2014 Journal of Cosmology and Astroparticle Physics
Planck 94
The Radiated Energy Budget of Chromospheric Plasma in a Major Solar Flare Deduced from Multi-wavelength Observations
DOI: 10.1088/0004-637X/793/2/70 Bibcode: 2014ApJ...793...70M

Chamberlin, Phillip C.; Milligan, Ryan O.; Kerr, Graham S. +7 more

This paper presents measurements of the energy radiated by the lower solar atmosphere, at optical, UV, and EUV wavelengths, during an X-class solar flare (SOL2011-02-15T01:56) in response to an injection of energy assumed to be in the form of nonthermal electrons. Hard X-ray observations from RHESSI were used to track the evolution of the paramete…

2014 The Astrophysical Journal
Hinode 94
Interstellar chemistry of nitrogen hydrides in dark clouds
DOI: 10.1051/0004-6361/201322386 Bibcode: 2014A&A...562A..83L

Maret, S.; Hily-Blant, P.; Pineau des Forêts, G. +3 more

Nitrogen, amongst the most abundant metals in the interstellar medium, has a peculiar chemistry that differs from those of carbon and oxygen. Recent observations of several nitrogen-bearing species in the interstellar medium suggest abundances in sharp disagreement with current chemical models. Although some of these observations show that some ga…

2014 Astronomy and Astrophysics
Herschel 94
Uncovering the Putative B-star Binary Companion of the SN 1993J Progenitor
DOI: 10.1088/0004-637X/790/1/17 Bibcode: 2014ApJ...790...17F

Van Dyk, Schuyler D.; Filippenko, Alexei V.; Chandra, Poonam +9 more

The Type IIb supernova (SN) 1993J is one of only a few stripped-envelope SNe with a progenitor star identified in pre-explosion images. SN IIb models typically invoke H envelope stripping by mass transfer in a binary system. For the case of SN 1993J, the models suggest that the companion grew to 22 M and became a source of ultraviolet…

2014 The Astrophysical Journal
eHST 94
A rapid decrease of the hydrogen corona of Mars
DOI: 10.1002/2014GL061803 Bibcode: 2014GeoRL..41.8013C

Quemerais, E.; Bertaux, J. -L.; Chaufray, J. -Y. +4 more

Mars is believed to have lost much of its surface water 3.5 billion years ago, but the amounts that escaped into space and remain frozen in the crust today are not well known. Hydrogen atoms in the extended martian atmosphere, some of which escape the planet's gravity, can be imaged through scattered solar UV radiation. Hubble Space Telescope (HST…

2014 Geophysical Research Letters
eHST 93
Weighing "El Gordo" with a Precision Scale: Hubble Space Telescope Weak-lensing Analysis of the Merging Galaxy Cluster ACT-CL J0102-4915 at z = 0.87
DOI: 10.1088/0004-637X/785/1/20 Bibcode: 2014ApJ...785...20J

Sifón, Cristóbal; Hughes, John P.; Barrientos, L. Felipe +5 more

We present a Hubble Space Telescope weak-lensing study of the merging galaxy cluster "El Gordo" (ACT-CL J0102-4915) at z = 0.87 discovered by the Atacama Cosmology Telescope (ACT) collaboration as the strongest Sunyaev-Zel'dovich decrement in its ~1000 deg2 survey. Our weak-lensing analysis confirms that ACT-CL J0102-4915 is indeed an e…

2014 The Astrophysical Journal
eHST 93
Rejecting Proposed Dense Matter Equations of State with Quiescent Low-mass X-Ray Binaries
DOI: 10.1088/2041-8205/796/1/L3 Bibcode: 2014ApJ...796L...3G

Guillot, Sebastien; Rutledge, Robert E.

Neutrons stars are unique laboratories for discriminating between the various proposed equations of state of matter at and above nuclear density. One sub-class of neutron stars—those inside quiescent low-mass X-ray binaries (qLMXBs)—produce a thermal surface emission from which the neutron star radius (R NS) can be measured, using the w…

2014 The Astrophysical Journal
XMM-Newton 93