Search Publications

Magnetic fluctuations embedded in dipolarization inside geosynchronous orbit and their associated selective acceleration of O+ ions
DOI: 10.1002/2014JA019806 Bibcode: 2014JGRA..119.4639N

Kistler, L. M.; Miyashita, Y.; Keika, K. +7 more

We study magnetic fluctuations embedded in dipolarizations in the inner magnetosphere (a geocentric distance of ≤6.6 RE) and their associated ion flux changes, using the Engineering Test Satellite VIII and Active Magnetospheric Particle Tracer Explorers/CCE satellites. We select seven events of dipolarization that occur during the main …

2014 Journal of Geophysical Research (Space Physics)
Cluster 26
Firm detection of a cyclotron resonance feature with Suzaku in the X-ray spectrum of GRO J1008-57 during a giant outburst in 2012
DOI: 10.1093/pasj/psu028 Bibcode: 2014PASJ...66...59Y

Makishima, Kazuo; Sasano, Makoto; Mihara, Tatehiro +3 more

We report on the firm detection of a cyclotron resonance scattering feature (CRSF) in the X-ray spectrum of the Be X-ray binary pulsar, GRO J1008-57, achieved by the Suzaku Hard X-ray Detector during a giant outburst which was detected by the MAXI Gas Slit Camera in 2012 November. The Suzaku observation was carried out on 2012 November 20, outburs…

2014 Publications of the Astronomical Society of Japan
Suzaku 26
The Taurus Boundary of Stellar/Substellar (TBOSS) Survey. I. Far-IR disk emission measured with Herschel
DOI: 10.1051/0004-6361/201323088 Bibcode: 2014A&A...570A..29B

Pinte, C.; Ménard, F.; Bouy, H. +4 more

With the PACS instrument on Herschel, 134 low mass members of the Taurus star-forming region spanning the M4-L0 spectral type range and covering the transition from low mass stars to brown dwarfs were observed. Combining the new Herschel results with other Herschel programs, a total of 150 of the 154 M4-L0 Taurus members have observations, and we …

2014 Astronomy and Astrophysics
Herschel eHST 26
Resolved Star Formation on Sub-galactic Scales in a Merger at z = 1.7
DOI: 10.1088/0004-637X/790/2/143 Bibcode: 2014ApJ...790..143W

Rigby, Jane R.; Whitaker, Katherine E.; Brammer, Gabriel B. +4 more

We present a detailed analysis of Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) G141 grism spectroscopy for seven star-forming regions of the highly magnified lensed starburst galaxy RCSGA 032727-132609 at z = 1.704. We measure the spatial variations of the extinction in RCS0327 through the observed Hγ/Hβ emission line ratios, finding a …

2014 The Astrophysical Journal
eHST 26
The average 0.5-200 keV spectrum of local active galactic nuclei and a new determination of the 2-10 keV luminosity function at z ≈ 0
DOI: 10.1093/mnras/stt2095 Bibcode: 2014MNRAS.437.2845B

Ballantyne, D. R.

The broad-band X-ray spectra of active galactic nuclei (AGNs) contains information about the nuclear environment from Schwarzschild radii scales (where the primary power law is generated in a corona) to distances of ∼1 pc (where the distant reflector may be located). In addition, the average shape of the X-ray spectrum is an important input into X…

2014 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 26
The Association of Solar Flares with Coronal Mass Ejections During the Extended Solar Minimum
DOI: 10.1007/s11207-013-0388-3 Bibcode: 2014SoPh..289.1257N

Lemen, J. R.; Aschwanden, M. J.; Nitta, N. V. +3 more

We study the association of solar flares with coronal mass ejections (CMEs) during the deep, extended solar minimum of 2007 - 2009, using extreme-ultraviolet (EUV) and white-light (coronagraph) images from the Solar Terrestrial Relations Observatory (STEREO). Although all of the fast (v>900 km s−1), wide (θ>100) CMEs a…

2014 Solar Physics
SOHO 26
Comparing supernova remnants around strongly magnetized and canonical pulsars
DOI: 10.1093/mnras/stu1594 Bibcode: 2014MNRAS.444.2910M

Rea, N.; Torres, D. F.; Martin, J. +1 more

The origin of the strong magnetic fields measured in magnetars is one of the main uncertainties in the neutron star field. On the other hand, the recent discovery of a large number of such strongly magnetized neutron stars is calling for more investigation on their formation. The first proposed model for the formation of such strong magnetic field…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 26
Half-megasecond Chandra Spectral Imaging of the Hot Circumgalactic Nebula around Quasar Mrk 231
DOI: 10.1088/0004-637X/790/2/116 Bibcode: 2014ApJ...790..116V

Maiolino, R.; Sturm, E.; Veilleux, S. +2 more

A deep 400 ks ACIS-S observation of the nearest quasar known, Mrk 231, is combined with archival 120 ks data to carry out the first ever spatially resolved spectral analysis of a hot X-ray-emitting circumgalactic nebula around a quasar. The 65 × 50 kpc X-ray nebula shares no resemblance with the tidal debris seen at optical wavelengths. One notabl…

2014 The Astrophysical Journal
eHST 26
Model-independent fit to Planck and BICEP2 data
DOI: 10.1103/PhysRevD.90.063007 Bibcode: 2014PhRvD..90f3007B

Mena, Olga; Barranco, Laura; Boubekeur, Lotfi

Inflation is the leading theory to describe elegantly the initial conditions that led to structure formation in our Universe. In this paper, we present a novel phenomenological fit to the Planck, WMAP polarization (WP) and the BICEP2 data sets using an alternative parametrization. Instead of starting from inflationary potentials and computing the …

2014 Physical Review D
Planck 26
An X-ray and UV flare from the galaxy XMMSL1 J061927.1-655311
DOI: 10.1051/0004-6361/201424347 Bibcode: 2014A&A...572A...1S

Read, A. M.; Esquej, P.; Komossa, S. +6 more


Aims: New high variability extragalactic sources may be identified by comparing the flux of sources seen in the XMM-Newton Slew Survey with detections and upper limits from the ROSAT All Sky Survey.
Methods: A detected flaring extragalactic source was monitored with Swift and XMM-Newton to track its temporal and spectral evolution. Optic…

2014 Astronomy and Astrophysics
XMM-Newton 26