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The HST/ACS Coma Cluster Survey - VI. Colour gradients in giant and dwarf early-type galaxies
DOI: 10.1111/j.1365-2966.2011.18606.x Bibcode: 2011MNRAS.414.3052D

Jogee, S.; Ferguson, H. C.; Peletier, R. F. +17 more

Using deep, high-spatial-resolution imaging from the Hubble Space Telescope/Advanced Camera for Surveys (HST/ACS) Coma Cluster Treasury Survey, we determine colour profiles of early-type galaxies in the Coma cluster. From 176 galaxies brighter than MF814W(AB)=-15 mag that are either spectroscopically confirmed members of Coma or identif…

2011 Monthly Notices of the Royal Astronomical Society
eHST 39
Altitude Distribution of the Auroral Acceleration Potential Determined from Cluster Satellite Data at Different Heights
DOI: 10.1103/PhysRevLett.106.055002 Bibcode: 2011PhRvL.106e5002M

Karlsson, Tomas; Fazakerley, Andrew; Nilsson, Hans +6 more

Aurora, commonly seen in the polar sky, is a ubiquitous phenomenon occurring on Earth and other solar system planets. The colorful emissions are caused by electron beams hitting the upper atmosphere, after being accelerated by quasistatic electric fields at 1-2 RE altitudes, or by wave electric fields. Although aurora was studied by man…

2011 Physical Review Letters
Cluster 39
Spectral and timing properties of the accreting X-ray millisecond pulsar IGR J17511-3057
DOI: 10.1051/0004-6361/201016240 Bibcode: 2011A&A...529A..68F

Stella, L.; Bozzo, E.; Kuiper, L. +6 more

Context. IGR J17511-3057 is the second X-ray transient accreting millisecond pulsar discovered by INTEGRAL. It was in outburst for about a month beginning on September 13, 2009.
Aims: We analyze the spectral and timing properties of the object and the characteristics of X-ray bursts with the aim to constrain the physical processes responsible…

2011 Astronomy and Astrophysics
INTEGRAL 39
Horizontal flow fields observed in Hinode G-band images. I. Methods
DOI: 10.1051/0004-6361/201016358 Bibcode: 2011A&A...529A.153V

Verma, M.; Denker, C.

Context. The interaction of plasma motions and magnetic fields is an important mechanism, which drives the solar activity in all its facets. For example, photospheric flows are responsible for the advection of magnetic flux, the redistribution of flux during the decay of sunspots, and the build-up of magnetic shear in flaring active regions.

2011 Astronomy and Astrophysics
Hinode 39
HIFI detection of hydrogen fluoride in the carbon star envelope IRC +10216
DOI: 10.1051/0004-6361/201117578 Bibcode: 2011A&A...533L...6A

Waters, L. B. F. M.; Teyssier, D.; Cernicharo, J. +5 more

We report the detection of emission in the J = 1-0 rotational transition of hydrogen fluoride (HF), together with observations of the J = 1-0 to J = 3-2 rotational lines of H35Cl and H37Cl, towards the envelope of the carbon star IRC +10216. High-sensitivity, high-spectral resolution observations have been carried out with th…

2011 Astronomy and Astrophysics
Herschel 39
Dynamics and circulation regimes of terrestrial planets
DOI: 10.1016/j.pss.2010.04.024 Bibcode: 2011P&SS...59..900R

Read, P. L.

By the study of simple analogues, either in the form of simplified numerical models or laboratory experiments, considerable insights may be gained as to the likely roles of planetary size, rotation, thermal stratification and other factors in determining the principal length scales, styles of global circulation and dominant waves and instability p…

2011 Planetary and Space Science
VenusExpress 39
Pre-flare Activity and Magnetic Reconnection during the Evolutionary Stages of Energy Release in a Solar Eruptive Flare
DOI: 10.1088/0004-637X/743/2/195 Bibcode: 2011ApJ...743..195J

Joshi, Bhuwan; Veronig, Astrid M.; Tiwari, Sanjiv Kumar +3 more

In this paper, we present a multi-wavelength analysis of an eruptive white-light M3.2 flare that occurred in active region NOAA 10486 on 2003 November 1. The excellent set of high-resolution observations made by RHESSI and the TRACE provides clear evidence of significant pre-flare activities for ~9 minutes in the form of an initiation phase observ…

2011 The Astrophysical Journal
SOHO 39
Fundamental Properties of the Highly Ionized Plasmas in the Milky Way
DOI: 10.1088/0004-637X/727/1/46 Bibcode: 2011ApJ...727...46L

Savage, B. D.; Lehner, N.; Howk, J. C. +1 more

The cooling transition temperature gas in the interstellar medium (ISM), traced by the high ions, Si IV, C IV, N V, and O VI, helps to constrain the flow of energy from the hot ISM with T>106 K to the warm ISM with T < 2 × 104 K. We investigate the properties of this gas along the lines of sight to 38 stars in the Milky…

2011 The Astrophysical Journal
eHST 39
Understanding the variability of nightside temperatures, NO UV and O2 IR nightglow emissions in the Venus upper atmosphere
DOI: 10.1029/2010JE003770 Bibcode: 2011JGRE..116.8004B

Gérard, J. -C.; Brecht, A. S.; Bougher, S. W. +3 more

Venus Express (VEX) has been monitoring key nightglow emissions and thermal features (O2 IR nightglow, NO UV nightglow, and nightside temperatures) which contribute to a comprehensive understanding of the global dynamics and circulation patterns above ∼90 km. The nightglow emissions serve as effective tracers of Venus' middle and upper …

2011 Journal of Geophysical Research (Planets)
VenusExpress 39
Evidence for Amazonian northern mid-latitude regional glacial landsystems on Mars: Glacial flow models using GCM-driven climate results and comparisons to geological observations
DOI: 10.1016/j.icarus.2011.07.018 Bibcode: 2011Icar..216...23F

Head, James W.; Forget, Francois; Fastook, James L. +2 more

A fretted valley system on Mars located at the northern mid-latitude dichotomy boundary contains lineated valley fill (LVF) with extensive flow-like features interpreted to be glacial in origin. We have modeled this deposit using glacial flow models linked to atmospheric general circulation models (GCM) for conditions consistent with the depositio…

2011 Icarus
MEx 39