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The First Measurement of the Adiabatic Index in the Solar Corona Using Time-dependent Spectroscopy of Hinode/EIS Observations
DOI: 10.1088/2041-8205/727/2/L32 Bibcode: 2011ApJ...727L..32V

Del Zanna, Giulio; Van Doorsselaere, Tom; Nakariakov, Valery M. +3 more

We use observations of a slow magnetohydrodynamic wave in the corona to determine for the first time the value of the effective adiabatic index, using data from the Extreme-ultraviolet Imaging Spectrometer on board Hinode. We detect oscillations in the electron density, using the CHIANTI atomic database to perform spectroscopy. From the time-depen…

2011 The Astrophysical Journal
Hinode 108
Galaxy stellar mass functions of different morphological types in clusters, and their evolution between z= 0.8 and 0
DOI: 10.1111/j.1365-2966.2010.17904.x Bibcode: 2011MNRAS.412..246V

Cava, Antonio; Fritz, Jacopo; Dressler, Alan +11 more

We present the galaxy stellar mass function and its evolution in clusters from z∼ 0.8 to the current epoch, based on the WIde-field Nearby Galaxy-cluster Survey (WINGS) (0.04 ≤z≤ 0.07), and the ESO Distant Cluster Survey (EDisCS) (0.4 ≤z≤ 0.8). We investigate the total mass function and find that it evolves noticeably with redshift. The shape at M…

2011 Monthly Notices of the Royal Astronomical Society
eHST 107
Measuring moonlight: An overview of the spatial properties, lunar coverage, selenolocation, and related Level 1B products of the Moon Mineralogy Mapper
DOI: 10.1029/2010JE003730 Bibcode: 2011JGRE..116.0G14B

Besse, S.; Isaacson, P.; Pieters, C. M. +7 more

The Moon Mineralogy Mapper (M3), a high-resolution, high-precision imaging spectrometer, flew on board India's Chandrayaan-1 Mission from October 2008 through August 2009. This paper describes some of the spatial sampling aspects of the instrument, the planned mission, and the mission as flown. We also outline the content and context of…

2011 Journal of Geophysical Research (Planets)
Chandrayaan-1 107
Two Components of the Solar Coronal Emission Revealed by Extreme-ultraviolet Spectroscopic Observations
DOI: 10.1088/0004-637X/738/1/18 Bibcode: 2011ApJ...738...18T

Martínez-Sykora, Juan; De Pontieu, Bart; Wang, Xin +3 more

Recent spectroscopic observations have revealed the ubiquitous presence of blueward asymmetries of emission lines formed in the solar corona and transition region. These asymmetries are most prominent in loop footpoint regions, where a clear correlation of the asymmetry with the Doppler shift and line width determined from the single-Gaussian fit …

2011 The Astrophysical Journal
Hinode 107
The Dark Matter Distribution in A383: Evidence for a Shallow Density Cusp from Improved Lensing, Stellar Kinematic, and X-ray Data
DOI: 10.1088/2041-8205/728/2/L39 Bibcode: 2011ApJ...728L..39N

Treu, Tommaso; Ellis, Richard S.; Newman, Andrew B. +1 more

We extend our analyses of the dark matter (DM) distribution in relaxed clusters to the case of A383, a luminous X-ray cluster at z = 0.189 with a dominant central galaxy and numerous strongly lensed features. Following our earlier papers, we combine strong and weak lensing constraints secured with Hubble Space Telescope and Subaru imaging with the…

2011 The Astrophysical Journal
eHST 107
Constraints on the Heating of High-temperature Active Region Loops: Observations from Hinode and the Solar Dynamics Observatory
DOI: 10.1088/0004-637X/734/2/90 Bibcode: 2011ApJ...734...90W

Winebarger, Amy R.; Warren, Harry P.; Brooks, David H.

We present observations of high-temperature emission in the core of a solar active region using instruments on Hinode and the Solar Dynamics Observatory (SDO). These multi-instrument observations allow us to determine the distribution of plasma temperatures and follow the evolution of emission at different temperatures. We find that at the apex of…

2011 The Astrophysical Journal
Hinode 107
Emission Lines from the Gas Disk around TW Hydra and the Origin of the Inner Hole
DOI: 10.1088/0004-637X/735/2/90 Bibcode: 2011ApJ...735...90G

Pascucci, I.; Najita, J.; Hollenbach, D. +1 more

We compare line emission calculated from theoretical disk models with optical to submillimeter wavelength observational data of the gas disk surrounding TW Hya and infer the spatial distribution of mass in the gas disk. The model disk that best matches observations has a gas mass ranging from ~10-4 to 10-5 M sun fo…

2011 The Astrophysical Journal
IUE 107
UV-to-FIR Analysis of Spitzer/IRAC Sources in the Extended Groth Strip. II. Photometric Redshifts, Stellar Masses, and Star Formation Rates
DOI: 10.1088/0067-0049/193/2/30 Bibcode: 2011ApJS..193...30B

Yamada, T.; Kajisawa, M.; Ashby, M. L. N. +6 more

Based on the ultraviolet to far-infrared photometry already compiled and presented in a companion paper (Paper I), we present a detailed spectral energy distribution (SED) analysis of nearly 80,000 IRAC 3.6 + 4.5 µm selected galaxies in the Extended Groth Strip. We estimate photometric redshifts, stellar masses, and star formation rates (SFR…

2011 The Astrophysical Journal Supplement Series
eHST 107
Fe-K Line Probing of Material Around the Active Galactic Nucleus Central Engine with Suzaku
DOI: 10.1088/0004-637X/727/1/19 Bibcode: 2011ApJ...727...19F

Fukazawa, Yasushi; Ohno, Masanori; Nishino, Sho +6 more

We systematically analyzed the high-quality Suzaku data of 88 Seyfert galaxies, about 31% of which are Compton-thick active galactic nuclei (AGNs). We obtained a clear relation between the absorption column density and the equivalent width (EW) of the 6.4 keV line above 1023 cm-2, suggesting a wide-ranging column density of 1…

2011 The Astrophysical Journal
Suzaku 107
Evidence for Cold Accretion: Primitive Gas Flowing onto a Galaxy at z ~ 0.274
DOI: 10.1088/0004-637X/743/2/207 Bibcode: 2011ApJ...743..207R

Tripp, Todd M.; Prochaska, J. Xavier; Lehner, Nicolas +5 more

We present UV and optical observations from the Cosmic Origins Spectrograph on the Hubble Space Telescope and Keck of a z = 0.27395 Lyman limit system (LLS) seen in absorption against the QSO PG1630+377. We detect H I absorption with log N(H I) = 17.06 ± 0.05 as well as Mg II, C III, Si III, and O VI in this system. The column densities are readil…

2011 The Astrophysical Journal
eHST 106