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Processing of Polycyclic Aromatic Hydrocarbons in Molecular-Loop Regions near the Galactic Center Revealed by AKARI
DOI: 10.1093/pasj/64.2.25 Bibcode: 2012PASJ...64...25K

Oyabu, Shinki; Onaka, Takashi; Yamagishi, Mitsuyoshi +7 more

We present an AKARI mid-infrared diffuse map of an area of about 4° × 3° near the Galactic center in the 9 µm band. The band intensity is mostly attributed to aromatic hydrocarbon infrared emissions of carbonaceous grains at wavelengths of 6.2, 7,7, 8.6, and 11.3 µm. We detected 9 µm emission structures extending from the Galacti…

2012 Publications of the Astronomical Society of Japan
AKARI 12
Flux transfer events: Motion and signatures
DOI: 10.1016/j.jastp.2011.07.010 Bibcode: 2012JASTP..87...20S

Omidi, N.; Sibeck, D. G.

We present results from a 2.5 dimensional hybrid code simulation for the evolution of flux transfer events (FTEs) during intervals of due southward interplanetary magnetic field (IMF) orientation. The structures invariably form between pairs of reconnection lines, often remaining nearly stationary on the subsolar magnetopause before their motion b…

2012 Journal of Atmospheric and Solar-Terrestrial Physics
Cluster 12
Axial symmetry breaking of Saturn's thermosphere
DOI: 10.1111/j.1365-2966.2012.20719.x Bibcode: 2012MNRAS.422.1460S

Achilleos, N.; Smith, C. G. A.

The source of the various planetary-period signals in Saturn's magnetosphere is at present unknown. We investigate the possibility that the source of these signals is an axially asymmetric wind system in the thermosphere. We describe a feedback mechanism that has the potential to drive such axially asymmetric wind systems. The proposed mechanism r…

2012 Monthly Notices of the Royal Astronomical Society
Cassini 12
Hunting for Young Dispersing Star Clusters in IC 2574
DOI: 10.1088/0004-6256/144/6/182 Bibcode: 2012AJ....144..182P

Pellerin, Anne; Harris, Jason; Meyer, Martin M. +1 more

Dissolving stellar groups are very difficult to detect using traditional surface photometry techniques. We have developed a method to find and characterize non-compact stellar systems in galaxies where the young stellar population can be spatially resolved. By carrying out photometry on individual stars, we are able to separate the luminous blue s…

2012 The Astronomical Journal
eHST 12
Velocity Characteristics of Rotating Sunspots
DOI: 10.1007/s11207-011-9923-2 Bibcode: 2012SoPh..278..121Z

Alexander, D.; Zhu, C.; Tian, L.

A statistical study is carried out to investigate the detailed relationship between rotating sunspots and the emergence of magnetic flux tubes. This paper presents the velocity characteristics of 132 sunspots in 95 solar active regions. The rotational characteristics of the sunspots are calculated from successive SOHO/MDI magnetograms by applying …

2012 Solar Physics
SOHO 12
Cassini VIMS Observations Show Ethane is Present in Titan's Rainfall
DOI: 10.1088/2041-8205/761/2/L24 Bibcode: 2012ApJ...761L..24D

Nicholson, Philip D.; Sotin, Christophe; Barnes, Jason W. +6 more

Observations obtained over two years by the Cassini Imaging Science Subsystem suggest that rain showers fall on the surface. Using measurements obtained by the Visual Infrared Mapping Spectrometer, we identify the main component of the rain to be ethane, with methane as an additional component. We observe five or six probable rainfall events, at l…

2012 The Astrophysical Journal
Cassini 12
The high-field polar RX J1007.5-2017
DOI: 10.1051/0004-6361/201219878 Bibcode: 2012A&A...546A.104T

Burwitz, V.; Beuermann, K.; Schwope, A. D. +2 more

We report optical and X-ray observations of the high-field polar RX J1007.5-2017 performed between 1990 and 2012. It has an orbital period of 208.60 min determined from the ellipsoidal modulation of the secondary star in an extended low state. The spectral flux of the dM3 - secondary star yields a distance of 790 ± 105 pc. At low accretion levels,…

2012 Astronomy and Astrophysics
XMM-Newton 12
Ongoing Massive Star Formation in NGC 604
DOI: 10.1088/0004-637X/761/1/3 Bibcode: 2012ApJ...761....3M

Groves, B.; Brandl, B.; Hunter, D. +1 more

NGC 604 is the second most massive H II region in the Local Group, thus an important laboratory for massive star formation. Using a combination of observational and analytical tools that include Spitzer spectroscopy, Herschel photometry, Chandra imaging, and Bayesian spectral energy distribution fitting, we investigate the physical conditions in N…

2012 The Astrophysical Journal
Herschel eHST 12
A Demonstration of Accurate Wide-field V-band Photometry Using a Consumer-grade DSLR Camera
DOI: 10.48550/arXiv.1303.6870 Bibcode: 2012JAVSO..40..815K

Maravelias, G.; Eggenstein, H. -B.; Kloppenborg, B. K. +2 more

The authors examined the suitability of using a Digital Single Lens Reflex (DSLR) camera for stellar photometry and, in particular, investigated wide field exposures made with minimal equipment for analysis of bright variable stars. A magnitude-limited sample of stars was evaluated exhibiting a wide range of (B-V) colors taken from four fields bet…

2012 Journal of the American Association of Variable Star Observers (JAAVSO)
Hipparcos 12
Light echo of V838 Monocerotis: properties of the echoing medium
DOI: 10.1051/0004-6361/201219858 Bibcode: 2012A&A...548A..23T

Tylenda, R.; Kamiński, T.

Context. The light echo phenomenon that accompanied the 2002 eruption of V838 Mon allows one to study the properties of the diffuse dusty matter in the vicinity of the object.
Aims: We are aiming at obtaining estimates of the optical thickness of the circumstellar matter in front of V838 Mon, as well as optical properties of dust grains in th…

2012 Astronomy and Astrophysics
eHST 12