Search Publications

A Simultaneous Forbush Decrease Associated with an Earthward Coronal Mass Ejection Observed by STEREO
DOI: 10.1007/s11207-012-0053-2 Bibcode: 2012SoPh..280..197O

Yi, Y.; Oh, S. Y.

The intensity-time profile of Forbush decrease (FD) events observed by neutron monitors (NMs) looks like that of a geomagnetic storm as defined by the Dst index. Oh, Yi, and Kim (J. Geophys. Res. 113, A01103, 2008) and Oh and Yi (J. Geophys. Res. 114, A11102, 2009) classified FD events based on the amount of overlap and simultaneity of their main …

2012 Solar Physics
SOHO 19
Evidence for Fresh Frost Layer on the Bare Nucleus of Comet Hale-Bopp at 32 AU Distance
DOI: 10.1088/0004-637X/761/1/8 Bibcode: 2012ApJ...761....8S

Pál, András; Sárneczky, Krisztián; Juhász, Attila +4 more

Here, we report that the activity of comet Hale-Bopp ceased between late 2007 and 2009 March, at about 28 AU distance from the Sun. At that time, the comet resided at a distance from the Sun that exceeded the freeze-out distance of regular comets by an order of magnitude. A Herschel Space Observatory PACS scan was taken in mid-2010, in the already…

2012 The Astrophysical Journal
Herschel eHST 19
Herschel and JCMT observations of the early-type dwarf galaxy NGC 205
DOI: 10.1111/j.1365-2966.2012.21044.x Bibcode: 2012MNRAS.423.2359D

Boquien, M.; Roussel, H.; Fritz, J. +18 more

We present Herschel dust continuum, James Clerk Maxwell Telescope CO (3-2) observations and a search for [C II] 158 ?m and [O I] 63 ?m spectral line emission for the brightest early-type dwarf satellite of Andromeda, NGC 205. While direct gas measurements [Mg∼ 1.5 × 106 M, H I+ CO (1-0)] have proven to be inconsis…

2012 Monthly Notices of the Royal Astronomical Society
Herschel 19
The XMM-Newton survey of the Small Magellanic Cloud: XMMU J010633.1-731543 and XMMU J010743.1-715953, two new Be/X-ray binary systems
DOI: 10.1111/j.1365-2966.2012.21193.x Bibcode: 2012MNRAS.424..282C

Haberl, F.; Hatzidimitriou, D.; Mereghetti, S. +6 more

In the course of the XMM-Newton survey of the Small Magellanic Cloud (SMC), two new bright X-ray sources were discovered exhibiting the spectral characteristics of high-mass X-ray binaries - but revealing only weak evidence for pulsations in just one of the objects (at 153 s in XMMU J010743.1-715953). The accurate X-ray source locations permit the…

2012 Monthly Notices of the Royal Astronomical Society
XMM-Newton 19
Ultraviolet Measurements of Interstellar C2
DOI: 10.1088/0004-637X/761/1/38 Bibcode: 2012ApJ...761...38H

Federman, S. R.; Sheffer, Y.; Hupe, Ryan C.

We analyzed archival spectra acquired with the Hubble Space Telescope for a study of interstellar C2. Absorption from the electronic transitions, D 1Σ+ u - X 1Σ+ g (0,0) as well as F 1Πu - X 1Σ+ g (0,0) and (1,0), was…

2012 The Astrophysical Journal
eHST 19
Estimates of Emission-Region Locations of Fermi Flat-Spectrum Radio Quasars
DOI: 10.1093/pasj/64.4.80 Bibcode: 2012PASJ...64...80Y

Zhang, Li; Yan, Dahai; Zeng, Houdun

We have studied the location of emission regions through modeling the quasi-simultaneous multifrequency spectral energy distributions of 21 Fermi flat-spectrum radio quasars (FSRQs) in the frame of a multicomponent one-zone leptonic model. In our calculations, we took the detailed broad line region (BLR) structure into account, and discussed the e…

2012 Publications of the Astronomical Society of Japan
Planck 19
New Evidence Supporting Cluster Membership for the Keystone Calibrator Delta Cephei
DOI: 10.1088/0004-637X/747/2/145 Bibcode: 2012ApJ...747..145M

Gieren, W.; Turner, D.; Majaess, D.

New and existing UBVJHKs , spectroscopic, NOMAD, Hubble Space Telescope, and revised Hipparcos observations are employed to determine properties for δ Cep and its host star cluster. The multi-faceted approach ensured that uncertainties were mitigated (σ/d ~ 2%). The following fundamental parameters were inferred for δ Cep: E(B - V) = 0.…

2012 The Astrophysical Journal
Hipparcos 19
Observations of Ionospheric Electron Beams in the Plasma Sheet
DOI: 10.1103/PhysRevLett.109.205001 Bibcode: 2012PhRvL.109t5001Z

Parks, G. K.; Fu, S. Y.; Pu, Z. Y. +3 more

Electrons streaming along the magnetic field direction are frequently observed in the plasma sheet of Earth’s geomagnetic tail. The impact of these field-aligned electrons on the dynamics of the geomagnetic tail is however not well understood. Here we report the first detection of field-aligned electrons with fluxes increasing at ∼1keV forming a “…

2012 Physical Review Letters
Cluster 19
Antitruncated stellar light profiles in the outer regions of STAGES spiral galaxies: bulge or disc related?
DOI: 10.1111/j.1365-2966.2011.20211.x Bibcode: 2012MNRAS.420.2475M

Wolf, Christian; Aragón-Salamanca, Alfonso; Hoyos, Carlos +2 more

We present a comparison of azimuthally averaged radial surface brightness µ(r) profiles and analytical bulge-disc decompositions (de Vaucouleurs, r1/4 bulge plus exponential disc) for spiral galaxies using Hubble Space Telescope/Advanced Camera for Surveys V-band imaging from the Space Telescope A901/2 Galaxy Evolution Survey (STA…

2012 Monthly Notices of the Royal Astronomical Society
eHST 19
Revealing the sub-structures of the magnetic reconnection separatrix via particle-in-cell simulation
DOI: 10.1063/1.4739283 Bibcode: 2012PhPl...19g2907Z

Deng, X. H.; Huang, S. Y.; Yuan, Z. G. +7 more

Magnetic separatrix is an important boundary layer separating the inflow and outflow regions in magnetic reconnection. In this article, we investigate the sub-structures of the separatrix region by using two-and-half dimensional electromagnetic particle-in-cell simulation. The separatrix region can be divided into two sub-regions in terms of the i…

2012 Physics of Plasmas
Cluster 19