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Suzaku Observation of the Fermi Cygnus Cocoon: The Search for a Signature of Young Cosmic-Ray Electrons
DOI: 10.1088/0004-637X/803/2/74 Bibcode: 2015ApJ...803...74M

Mizuno, T.; Takahashi, H.; Tibaldo, L. +4 more

The origin of Galactic cosmic rays remains unconfirmed, but promising candidates for their sources are found in star-forming regions. We report a series of X-ray observations, with Suzaku, toward the nearby star-forming region of Cygnus X. They aim at comparing diffuse X-ray emissions on and off the γ-ray cocoon of hard cosmic rays revealed by the…

2015 The Astrophysical Journal
Suzaku 10
Chromospheric Rapid Blueshifted Excursions Observed with IBIS and their Association with Photospheric Magnetic Field Evolution
DOI: 10.1088/0004-637X/799/2/219 Bibcode: 2015ApJ...799..219D

Liu, Chang; Jing, Ju; Denker, Carsten +9 more

Chromospheric rapid blueshifted excursions (RBEs) are suggested to be the disk counterparts of type II spicules at the limb and believed to contribute to the coronal heating process. Previous identification of RBEs was mainly based on feature detection using Dopplergrams. In this paper, we study RBEs on 2011 October 21 in a very quiet region at th…

2015 The Astrophysical Journal
Hinode 10
Constraints on the Surface Magnetic Fields and Age of a Cool Hypergiant: XMM-Newton X-Ray Observations of VY CMa
DOI: 10.1088/0004-637X/800/1/4 Bibcode: 2015ApJ...800....4M

Humphreys, Roberta M.; Davidson, Kris; Kastner, Joel H. +2 more

The complex circumstellar ejecta of highly evolved, cool hypergiants are indicative of multiple, asymmetric mass-loss events. To explore whether such episodic, non-isotropic mass loss may be driven by surface magnetic activity, we have observed the archetypical cool hypergiant VY CMa with the XMM-Newton X-ray satellite observatory. The hypergiant …

2015 The Astrophysical Journal
XMM-Newton 9
A Tale of Three Mysterious Spectral Features in Carbon-rich Evolved Stars: The 21 µm, 30 µm, and “Unidentified Infrared” Emission Features
DOI: 10.1088/0004-637X/802/1/39 Bibcode: 2015ApJ...802...39M

Li, Aigen; Jiang, B. W.; Mishra, Ajay

The mysterious “21 µm” emission feature seen almost exclusively in the short-lived protoplanetary nebula (PPN) phase of stellar evolution remains unidentified since its discovery two decades ago. This feature is always accompanied by the equally mysterious, unidentified “30 µm” feature and the so-called “unidentified infrared” (UIR) fe…

2015 The Astrophysical Journal
ISO 9
Re-evaluation of the Neutron Emission from the Solar Flare of 2005 September 7, Detected by the Solar Neutron Telescope at Sierra Negra
DOI: 10.1088/0004-637X/814/2/136 Bibcode: 2015ApJ...814..136G

Watanabe, K.; Matsubara, Y.; Muraki, Y. +9 more

The X17.0 solar flare of 2005 September 7 released high-energy neutrons that were detected by the Solar Neutron Telescope (SNT) at Sierra Negra, Mexico. In three separate and independent studies of this solar neutron event, several of its unique characteristics were studied; in particular, a power-law energy spectra was estimated. In this paper, w…

2015 The Astrophysical Journal
INTEGRAL 9
Plasma Physical Parameters along CME-driven Shocks. II. Observation-Simulation Comparison
DOI: 10.1088/0004-637X/809/1/58 Bibcode: 2015ApJ...809...58B

Bemporad, A.; Susino, R.; Lapenta, G. +1 more

In this work, we compare the spatial distribution of the plasma parameters along the 1999 June 11 coronal mass ejection (CME)-driven shock front with the results obtained from a CME-like event simulated with the FLIPMHD3D code, based on the FLIP-MHD particle-in-cell method. The observational data are retrieved from the combination of white-light c…

2015 The Astrophysical Journal
SOHO 9
Herschel Dust Emission as a Probe of Starless Cores Mass: MCLD 123.5+24.9 of the Polaris Flare
DOI: 10.1088/0004-637X/809/1/17 Bibcode: 2015ApJ...809...17W

Ferland, Gary J.; Abel, Nicholas P.; Wagle, Gururaj A. +1 more

We present newly processed archival Herschel images of molecular cloud MCLD 123.5+24.9 in the Polaris Flare. This cloud contains five starless cores. Using the spectral synthesis code Cloudy, we explore uncertainties in the derivation of column densities, and hence masses of molecular cores from Herschel data. We first consider several detailed gr…

2015 The Astrophysical Journal
Herschel 9
X-Ray Perspective of the Twisted Magnetospheres of Magnetars
DOI: 10.1088/0004-637X/805/1/81 Bibcode: 2015ApJ...805...81W

Göğüş, Ersin; Weng, Shan-Shan; Lin, Lin +1 more

Anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs) are recognized as the most promising magnetar candidates, as indicated by their energetic bursts and rapid spin-downs. It is expected that the strong magnetic field leaves distinctive imprints on the emergent radiation both by affecting the radiative processes in atmospheres of mag…

2015 The Astrophysical Journal
XMM-Newton 9
Far-ultraviolet Study of the ζ-Ophiuchi H II Region
DOI: 10.1088/0004-637X/800/2/132 Bibcode: 2015ApJ...800..132C

Choi, Yeon-Ju; Min, Kyoung-Wook; Seon, Kwang-Il

We report the results of our analysis of the H II region around ζ Oph based on far-ultraviolet (FUV) spectral imaging observations, together with data made in other wavelengths. We found that scattering by dust grains of the FUV photons, which originate mostly from ζ Oph, dominates the FUV emission in this region, while contributions from the two-…

2015 The Astrophysical Journal
IUE 9
Detection of a Compact Nuclear Radio Source in the Local Group Elliptical Galaxy M32
DOI: 10.1088/2041-8205/807/1/L19 Bibcode: 2015ApJ...807L..19Y

Wang, Q. Daniel; Kraft, Ralph P.; Li, Zhiyuan +4 more

The Local Group compact elliptical galaxy M32 hosts one of the nearest candidate supermassive black holes (SMBHs), which has a previously suggested X-ray counterpart. Based on sensitive observations taken with the Karl G. Jansky Very Large Array (VLA), we detect for the first time a compact radio source coincident with the nucleus of M32, which ex…

2015 The Astrophysical Journal
XMM-Newton eHST 9