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New Solar Telescope Observations of Magnetic Reconnection Occurring in the Chromosphere of the Quiet Sun
DOI: 10.1088/2041-8205/713/1/L6 Bibcode: 2010ApJ...713L...6C

Chae, Jongchul; Goode, P. R.; Ahn, K. +5 more

Magnetic reconnection is a process in which field-line connectivity changes in a magnetized plasma. On the solar surface, it often occurs with the cancellation of two magnetic fragments of opposite polarity. Using the 1.6 m New Solar Telescope, we observed the morphology and dynamics of plasma visible in the Hα line, which is associated with a can…

2010 The Astrophysical Journal
SOHO 21
Toward the General Red Giant Branch Slope-Metallicity-Age Calibration. I. Metallicities, Ages, and Kinematics for Eight Large Magellanic Cloud Clusters
DOI: 10.1088/0004-6256/139/3/878 Bibcode: 2010AJ....139..878S

Geisler, D.; Sharma, Saurabh; Borissova, J. +2 more

In this paper, we discuss the properties of color-magnitude diagrams, age, metallicity, and radial velocities of eight massive Large Magellanic Cloud (LMC) clusters using data taken from the FORS2 multiobject spectrograph at the 8.2 m Very Large Telescope/Unit Telescope 1. The strong near-infrared Ca II triplet lines of red giant branch stars obta…

2010 The Astronomical Journal
eHST 21
A Novel Approach in Constraining Electron Spectra in Blazar Jets: The Case of Markarian 421
DOI: 10.1088/0004-637X/724/2/1509 Bibcode: 2010ApJ...724.1509U

Takahashi, Tadayuki; Tanaka, Takaaki; Kataoka, Jun +7 more

We report results from the observations of the well-studied TeV blazar Mrk 421 with the Swift and the Suzaku satellites in 2008 December. During the observation, Mrk 421 was found in a relatively low activity state, with the corresponding 2-10 keV flux of 3 × 10-10 erg s-1 cm-2. For the purpose of robustly constrai…

2010 The Astrophysical Journal
Suzaku 21
Suzaku Observations of the Black Hole H1743-322 in Outburst
DOI: 10.1088/0004-637X/713/2/1244 Bibcode: 2010ApJ...713.1244B

Yamaoka, K.; Takahashi, H.; Fabian, A. C. +5 more

We observed the Galactic black hole candidate H1743-322 with Suzaku for approximately 32 ks, while the source was in a low/hard state during its 2008 outburst. We collected and analyzed the data with the HXD/PIN, HXD/GSO, and XIS cameras spanning the energy range 0.7-200 keV. Fits to the spectra with simple models fail to detect narrow Fe XXV and …

2010 The Astrophysical Journal
Suzaku 21
Gas kinetics and dust dynamics in low-density comet comae
DOI: 10.1016/j.icarus.2010.06.022 Bibcode: 2010Icar..210..455D

Kamp, Lucas; Gulkis, Samuel; Lee, Seungwon +4 more

Extensive regions of low-density cometary comae are characterized by important deviations from the Maxwell-Boltzmann velocity distribution, i.e. breakdown of thermodynamic equilibrium. The consequences of this on the shapes of emission and absorption lines, and for the acceleration of solid bodies due to gas drag, have rarely been investigated. Th…

2010 Icarus
Rosetta 21
The warm absorber and X-ray variability of the Seyfert 1 galaxy NGC 3516 as seen by the XMM-Newton RGS
DOI: 10.1051/0004-6361/200913049 Bibcode: 2010A&A...514A.100M

Mehdipour, M.; Page, M. J.; Branduardi-Raymont, G.


Aims: We present a new analysis of the soft and medium energy X-ray spectrum of the Seyfert 1 galaxy NGC 3516 taken with the Reflection Grating Spectrometer (RGS) and European Photon Imaging Camera (EPIC) on board the XMM-Newton observatory. We examine four observations made in October 2006. We investigate whether the observed variability is …

2010 Astronomy and Astrophysics
XMM-Newton 21
Field and Globular Cluster Low-mass X-ray Binaries in NGC 4278
DOI: 10.1088/0004-637X/725/2/1824 Bibcode: 2010ApJ...725.1824F

Zezas, A.; Gallagher, J.; King, A. R. +12 more

We report a detailed spectral analysis of the population of low-mass X-ray binaries (LMXBs) detected in the elliptical galaxy NGC 4278 with Chandra. Seven luminous sources were studied individually, four in globular clusters (GCs) and three in the stellar field. The range of (0.3-8 keV) L X for these sources is ~(3-8) × 1038

2010 The Astrophysical Journal
eHST 21
The Discovery of Infrared Rings in the Planetary Nebula NGC 1514 During the WISE All-sky Survey
DOI: 10.1088/0004-6256/140/6/1882 Bibcode: 2010AJ....140.1882R

Hoard, D. W.; Wright, Edward L.; Wachter, Stefanie +3 more

We report the discovery of a pair of infrared, axisymmetric rings in the planetary nebula NGC 1514 during the course of the WISE all-sky mid-infrared survey. Similar structures are seen at visible wavelengths in objects such as the "Engraved Hourglass Nebula" (MyCn 18) and the "Southern Crab Nebula" (Hen 2-104). However, in NGC 1514 we see only a …

2010 The Astronomical Journal
ISO 21
Galaxy Clusters at z >= 1: Gas Constraints from the Sunyaev-Zel'dovich Array
DOI: 10.1088/2041-8205/723/1/L78 Bibcode: 2010ApJ...723L..78C

Andreon, S.; Carlstrom, J. E.; Leitch, E. M. +20 more

We present gas constraints from Sunyaev-Zel'dovich (SZ) effect measurements in a sample of 11 X-ray and infrared (IR) selected galaxy clusters at z>=1, using data from the Sunyaev-Zel'dovich Array (SZA). The cylindrically integrated Compton-y parameter, Y, is calculated by fitting the data to a two-parameter gas pressure profile. Where possible…

2010 The Astrophysical Journal
XMM-Newton 21
Ground-state ammonia and water in absorption towards Sgr B2
DOI: 10.1051/0004-6361/200913766 Bibcode: 2010A&A...522A..19W

Falgarone, E.; Larsson, B.; Olberg, M. +8 more

Context. Observations of transitions to the ground-state of a molecule are essential to obtain a complete picture of its excitation and chemistry in the interstellar medium, especially in diffuse and/or cold environments. For the important interstellar molecules H2O and NH3, these ground-state transitions are heavily absorbed…

2010 Astronomy and Astrophysics
ISO 21