Search Publications

Tightening the belt: Constraining the mass and evolution in SDC335
DOI: 10.1051/0004-6361/201425041 Bibcode: 2015A&A...577A..30A

Avison, A.; Peretto, N.; Fuller, G. A. +3 more


Aims: Recent ALMA observations identified one of the most massive star-forming cores yet observed in the Milky Way: SDC335-MM1, within the infrared dark cloud SDC335.579-0.292. Along with an accompanying core MM2, SDC335 appears to be in the early stages of its star formation process. We aim to constrain the properties of the stars forming wi…

2015 Astronomy and Astrophysics
Herschel 17
Recent highlights from Cluster, the first 3-D magnetospheric mission
DOI: 10.5194/angeo-33-1221-2015 Bibcode: 2015AnGeo..33.1221E

Escoubet, C. P.; Goldstein, M. L.; Masson, A. +1 more

The Cluster mission has been operated successfully for 14 years. During this time period, the evolution of the orbit has enabled Cluster to sample many more magnetospheric regions than was initially anticipated. So far, the separation of the Cluster spacecraft has been changed more than 30 times and has ranged from a few kilometres up to 36 000 km…

2015 Annales Geophysicae
Cluster 17
Constraining dark sector perturbations I: cosmic shear and CMB lensing
DOI: 10.1088/1475-7516/2015/04/048 Bibcode: 2015JCAP...04..048B

Battye, Richard A.; Moss, Adam; Pearson, Jonathan A.

We present current and future constraints on equations of state for dark sector perturbations. The equations of state considered are those corresponding to a generalized scalar field model and time-diffeomorphism invariant ℒ(g) theories that are equivalent to models of a relativistic elastic medium and also Lorentz violating massive gravity. We de…

2015 Journal of Cosmology and Astroparticle Physics
Planck 17
Suzaku observation of Be/X-ray binary pulsar EXO 2030+375
DOI: 10.1088/1674-4527/15/4/007 Bibcode: 2015RAA....15..537N

Naik, Sachindra; Jaisawal, Gaurava K.

We study the timing and spectral properties of Be/X-ray binary pulsar EXO 2030+375 using a Suzaku observation taken on 2012 May 23, during a less intense Type I outburst. Pulsations were clearly detected in the X-ray light curves at a barycentric period of 41.2852 s, which suggest that the pulsar is spinning-up. The pulse profiles were found to be…

2015 Research in Astronomy and Astrophysics
Suzaku 17
Signature of the presence of a third body orbiting around XB 1916-053
DOI: 10.1051/0004-6361/201526500 Bibcode: 2015A&A...582A..32I

Sanna, A.; Romano, P.; Di Salvo, T. +9 more

Context. The ultra-compact dipping source XB 1916-053 has an orbital period of close to 50 min and a companion star with a very low mass (less than 0.1 M). The orbital period derivative of the source was estimated to be 1.5(3) × 10-11 s/s through analysing the delays associated with the dip arrival times o…

2015 Astronomy and Astrophysics
Exosat INTEGRAL XMM-Newton 17
Cosmic microwave background anisotropies in the timescape cosmology
DOI: 10.1103/PhysRevD.91.063519 Bibcode: 2015PhRvD..91f3519N

Wiltshire, David L.; Nazer, M. Ahsan

We analyze the spectrum of cosmic microwave background (CMB) anisotropies in the timescape cosmology: a potentially viable alternative to homogeneous isotropic cosmologies without dark energy. We exploit the fact that the timescape cosmology is extremely close to the standard cosmology at early epochs to adapt existing numerical codes to produce C…

2015 Physical Review D
Planck 17
Detection of fundamental and first harmonic cyclotron line in X-ray pulsar Cep X-4
DOI: 10.1093/mnrasl/slv093 Bibcode: 2015MNRAS.453L..21J

Naik, Sachindra; Jaisawal, Gaurava K.

We report the broad-band spectral properties of the X-ray pulsar Cep X-4 by using a Suzaku observation in 2014 July. The 0.8-70 keV spectrum was found to be well described by three continuum models - Negative and Positive power-law with Exponential cut-off (NPEX), high-energy cut-off power-law and CompTT models. Additional components such as a cyc…

2015 Monthly Notices of the Royal Astronomical Society
Suzaku 17
X-Ray Fading and Expansion in the “Miniature Supernova Remnant” of GK Persei
DOI: 10.1088/0004-637X/801/2/92 Bibcode: 2015ApJ...801...92T

Yamaguchi, H.; Uchiyama, Y.; Drake, J. J. +3 more

We report on a second epoch of Chandra X-ray imaging spectroscopy of the spatially resolved old nova remnant GK Persei. An ACIS-S3 observation of 97.4 ks was conducted in 2013 November after a lapse of 13.8 yr from the last visit in 2000. The X-ray emitting nebula appeared more faint and patchy compared with the first epoch. The flux decline was p…

2015 The Astrophysical Journal
eHST 17
Spatial distribution of ice blocks on Enceladus and implications for their origin and emplacement
DOI: 10.1016/j.icarus.2014.09.035 Bibcode: 2015Icar..245..162M

Ingersoll, Andrew P.; Ewald, Shawn P.; Helfenstein, Paul +2 more

We have mapped the locations of over 100,000 ice blocks across the south polar region of Saturn's moon Enceladus, thus generating the first quantitative estimates of ice-block number density distribution in relation to major geological features. Ice blocks were manually identified and mapped from twenty of the highest resolution (4-25 m per pixel)…

2015 Icarus
Cassini 17
Wave-like Formation of Hot Loop Arcades
DOI: 10.1007/s11207-015-0769-x Bibcode: 2015SoPh..290.2909R

Shestov, S.; Kuzin, S.; Zimovets, I. +2 more

We present observations of hot arcades made with the Mg XII spectroheliograph onboard the CORONAS-F mission, which provides monochromatic images of hot plasma in the Mg XII 8.42 Å resonance line. The arcades were observed to form above the polarity inversion line between active regions NOAA 09847 and 09848 at four successive episodes: at 09:18, 14…

2015 Solar Physics
SOHO 17