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Stellar clusters in M83: formation, evolution, disruption and the influence of the environment
DOI: 10.1111/j.1365-2966.2011.19909.x Bibcode: 2012MNRAS.419.2606B

Bastian, N.; Larsen, S. S.; Smith, L. J. +6 more

We study the stellar cluster population in two adjacent fields in the nearby, face-on spiral galaxy M83 using multiwavelength Wide Field Camera 3/Hubble Space Telescope imaging. After automatic detection procedures, the clusters are selected through visual inspection to be centrally concentrated, symmetric, and resolved on the images, which allows…

2012 Monthly Notices of the Royal Astronomical Society
eHST 153
Occurrence rate of earthward-propagating dipolarization fronts
DOI: 10.1029/2012GL051784 Bibcode: 2012GeoRL..3910101F

André, M.; Vaivads, A.; Huang, S. Y. +2 more

The occurrence rate of earthward-propagating dipolarization fronts (DFs) is investigated in this paper based on the 9 years (2001-2009) of Cluster 1 data. For the first time, we select the DF events by fitting the characteristic increase in Bz using a hyperbolic tangent function. 303 earthward-propagating DFs are found; they have on ave…

2012 Geophysical Research Letters
Cluster 153
Faint high-redshift AGN in the Chandra deep field south: the evolution of the AGN luminosity function and black hole demography
DOI: 10.1051/0004-6361/201117581 Bibcode: 2012A&A...537A..16F

Pannella, M.; Fiore, F.; Castellano, M. +14 more

Context. We present detection and analysis of faint X-ray sources in the Chandra deep field south (CDFS) using the 4 Ms Chandra observation.
Aims: We place constraints on active galactic nuclei (AGN) luminosity functions at z = 3-7, its cosmological evolution, and high-redshift black hole and AGN demography.
Methods: We use a new detecti…

2012 Astronomy and Astrophysics
eHST 152
Investigations of dust heating in M81, M83 and NGC 2403 with the Herschel Space Observatory
DOI: 10.1111/j.1365-2966.2011.19735.x Bibcode: 2012MNRAS.419.1833B

Clements, D. L.; Roussel, H.; Cooray, A. +21 more

We use Spitzer Space Telescope and Herschel Space Observatory far-infrared data along with ground-based optical and near-infrared data to understand how dust heating in the nearby face-on spiral galaxies M81, M83 and NGC 2403 is affected by the starlight from all stars and by the radiation from star-forming regions. We find that 70/160 ?m surface …

2012 Monthly Notices of the Royal Astronomical Society
Herschel 152
Quantifying Spicules
DOI: 10.1088/0004-637X/759/1/18 Bibcode: 2012ApJ...759...18P

De Pontieu, Bart; Carlsson, Mats; Pereira, Tiago M. D.

Understanding the dynamic solar chromosphere is fundamental in solar physics. Spicules are an important feature of the chromosphere, connecting the photosphere to the corona, potentially mediating the transfer of energy and mass. The aim of this work is to study the properties of spicules over different regions of the Sun. Our goal is to investiga…

2012 The Astrophysical Journal
Hinode 152
Disentangling Baryons and Dark Matter in the Spiral Gravitational Lens B1933+503
DOI: 10.1088/0004-637X/750/1/10 Bibcode: 2012ApJ...750...10S

McKean, J. P.; Treu, T.; Auger, M. W. +10 more

Measuring the relative mass contributions of luminous and dark matter in spiral galaxies is important for understanding their formation and evolution. The combination of a galaxy rotation curve and strong lensing is a powerful way to break the disk-halo degeneracy that is inherent in each of the methods individually. We present an analysis of the …

2012 The Astrophysical Journal
eHST 152
Neutral Interstellar Helium Parameters Based on IBEX-Lo Observations and Test Particle Calculations
DOI: 10.1088/0067-0049/198/2/12 Bibcode: 2012ApJS..198...12B

Bochsler, P.; McComas, D. J.; Fuselier, S. A. +10 more

Because of its high ionization potential and weak interaction with hydrogen, neutral interstellar helium (NISHe) is almost unaffected at the heliospheric interface with the interstellar medium and freely enters the solar system. This second most abundant species provides some of the best information on the characteristics of the interstellar gas i…

2012 The Astrophysical Journal Supplement Series
Ulysses 151
The Large Longitudinal Spread of Solar Energetic Particles During the 17 January 2010 Solar Event
DOI: 10.1007/s11207-012-0049-y Bibcode: 2012SoPh..281..281D

Gómez-Herrero, R.; Dresing, N.; Heber, B. +3 more

We investigate multi-spacecraft observations of the 17 January 2010 solar energetic particle event. Energetic electrons and protons have been observed over a remarkable large longitudinal range at the two STEREO spacecraft and SOHO, suggesting a longitudinal spread of nearly 360 degrees at 1 AU. The flaring active region, which was on the backside…

2012 Solar Physics
SOHO 150
Dwarfs Gobbling Dwarfs: A Stellar Tidal Stream around NGC 4449 and Hierarchical Galaxy Formation on Small Scales
DOI: 10.1088/2041-8205/748/2/L24 Bibcode: 2012ApJ...748L..24M

Carballo-Bello, Julio A.; Romanowsky, Aaron J.; Brodie, Jean P. +13 more

A candidate diffuse stellar substructure was previously reported in the halo of the nearby dwarf starburst galaxy NGC 4449 by Karachentsev et al. We map and analyze this feature using a unique combination of deep integrated-light images from the BlackBird 0.5 m telescope, and high-resolution wide-field images from the 8 m Subaru Telescope, which r…

2012 The Astrophysical Journal
eHST 149
Hubble Space Telescope Reveals Multiple Sub-giant Branch in Eight Globular Clusters
DOI: 10.1088/0004-637X/760/1/39 Bibcode: 2012ApJ...760...39P

Anderson, J.; Milone, A. P.; Marino, A. F. +6 more

In the last few years many globular clusters (GCs) have revealed complex color-magnitude diagrams, with the presence of multiple main sequences (MSs), broad or multiple sub-giant branches (SGBs) and MS turnoffs, and broad or split red giant branches (RGBs). After a careful correction for differential reddening, high-accuracy photometry with the Hu…

2012 The Astrophysical Journal
eHST 149