Search Publications

The Mass-Lx Relation for Moderate Luminosity X-ray Clusters
DOI: 10.1088/0004-637X/726/1/48 Bibcode: 2011ApJ...726...48H

McNamara, Brian R.; Donahue, Megan; Voit, G. Mark +2 more

We present measurements of the masses of a sample of 25 moderate X-ray luminosity clusters of galaxies from the 160 square degree ROSAT survey. The masses were obtained from a weak-lensing analysis of deep F814W images obtained using the Advanced Camera for Surveys. We present an accurate empirical correction for the effect of charge transfer (in)…

2011 The Astrophysical Journal
eHST 41
Hubble Space Telescope Imaging of Lyα Emission at z ≈ 4.4
DOI: 10.1088/0004-637X/735/1/5 Bibcode: 2011ApJ...735....5F

Finkelstein, Steven L.; Grogin, Norman A.; Hathi, Nimish P. +28 more

We present the highest redshift detections of resolved Lyα emission, using Hubble Space Telescope (HST)/Advanced Camera for Surveys F658N narrowband-imaging data taken in parallel with the Wide Field Camera 3 Early Release Science program in the GOODS Chandra Deep Field-South. We detect Lyα emission from three spectroscopically confirmed z = 4.4 L…

2011 The Astrophysical Journal
eHST 41
Different Patterns of Chromospheric Evaporation in a Flaring Region Observed with Hinode/EIS
DOI: 10.1088/0004-637X/727/2/98 Bibcode: 2011ApJ...727...98L

Ding, M. D.; Li, Y.

We investigate the chromospheric evaporation in the flare of 2007 January 16 using line profiles observed by the Exterme-UV Imaging Spectrometer on board Hinode. Three points at flare ribbons of different magnetic polarities are analyzed in detail. We find that the three points show different patterns of upflows and downflows in the impulsive phas…

2011 The Astrophysical Journal
Hinode SOHO 41
Did the Sun Change Its Behaviour During the Decline of Cycle 23 and Into Cycle 24?
DOI: 10.1007/s11207-011-9827-1 Bibcode: 2011SoPh..272..337T

Tapping, K. F.; Valdés, J. J.

The activity minimum between the end of cycle 23 and the beginning of cycle 24 was the longest and deepest since at least the beginning of the 20th century. This has led to speculation that the Sun is changing its behaviour. The sunspot number and 10.7-cm solar radio flux indices have traditionally been highly correlated, so a change in the relati…

2011 Solar Physics
SOHO 41
Can coronal hole spicules reach coronal temperatures?
DOI: 10.1051/0004-6361/201116735 Bibcode: 2011A&A...532L...1M

Doyle, J. G.; Madjarska, M. S.; Vanninathan, K.


Aims: The present study aims to provide observational evidence of whether coronal hole spicules reach coronal temperatures.
Methods: We combine multi-instrument co-observations obtained with the SUMER/SoHO and with the EIS/SOT/XRT/Hinode.
Results: The analysed three large spicules were found to be comprised of numerous thin spicules…

2011 Astronomy and Astrophysics
Hinode SOHO 41
A mid-IR study of Hickson compact groups. II. Multiwavelength analysis of the complete GALEX-Spitzer sample
DOI: 10.1051/0004-6361/201117355 Bibcode: 2011A&A...533A.142B

Le Floc'h, E.; Magdis, G.; da Cunha, E. +3 more

We present a comprehensive study of the impact of the environment of compact galaxy groups on the evolution of their members using a multiwavelength analysis from the ultraviolet to the infrared, for a sample of 32 Hickson compact groups (HCGs) containing 135 galaxies. Fitting the spectral energy distributions (SEDs) of all galaxies with the state…

2011 Astronomy and Astrophysics
AKARI 41
Long-term spectral and timing properties of the soft gamma-ray repeater SGR 1833-0832 and detection of extended X-ray emission around the radio pulsar PSR B1830-08
DOI: 10.1111/j.1365-2966.2011.19022.x Bibcode: 2011MNRAS.416..205E

Sakamoto, T.; Wieringa, M. H.; Tiengo, A. +19 more

SGR 1833-0832 was discovered on 2010 March 19, thanks to the Swift detection of a short hard X-ray burst and follow-up X-ray observations. Since then, it was repeatedly observed with Swift, Rossi X-ray Timing Explorer and XMM-Newton. Using these data, which span about 225 d, we studied the long-term spectral and timing characteristics of SGR 1833-…

2011 Monthly Notices of the Royal Astronomical Society
XMM-Newton 41
Evolution of sunspot properties during solar cycle 23
DOI: 10.1051/0004-6361/201116655 Bibcode: 2011A&A...533A..14W

Fletcher, L.; Marshall, S.; Watson, F. T.

Context. The long term study of the Sun is necessary if we are to determine the evolution of sunspot properties and thereby inform modeling of the solar dynamo, particularly on scales of a solar cycle.
Aims: We aim to determine a number of sunspot properties over cycle 23 using the uniform database provided by the SOHO Michelson Doppler Image…

2011 Astronomy and Astrophysics
SOHO 41
The Solar Energetic Balance Revisited by Young Solar Analogs, Helioseismology, and Neutrinos
DOI: 10.1088/2041-8205/731/2/L29 Bibcode: 2011ApJ...731L..29T

Turck-Chièze, Sylvaine; Couvidat, Sébastien; Piau, Laurent

The energetic balance of the standard solar model (SSM) results from equilibrium between nuclear energy production, energy transfer, and photospheric emission. In this Letter, we give an order of magnitude of several percent for the loss of energy in kinetic energy, magnetic energy, and X-ray or UV radiation during the entire solar lifetime from t…

2011 The Astrophysical Journal
SOHO 41
Sympathetic Filament Eruptions Connected by Coronal Dimmings
DOI: 10.1088/0004-637X/738/2/179 Bibcode: 2011ApJ...738..179J

Yang, Jiayan; Bi, Yi; Hong, Junchao +2 more

We present for the first time detailed observations of three successive, interdependent filament eruptions that occurred one by one within 5 hr from different locations beyond the range of a single active region. The first eruption was observed from an active region and was associated with a coronal mass ejection (CME), during which diffuse and co…

2011 The Astrophysical Journal
SOHO 41