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NGC 2419: a large and extreme second generation in a currently undisturbed cluster
DOI: 10.1111/j.1365-2966.2011.18642.x Bibcode: 2011MNRAS.414.3381D

Milone, A. P.; D'Antona, F.; Ventura, P. +6 more

We analyse complementary Hubble Space Telescope and Subaru data for the globular cluster NGC 2419. We make a detailed analysis of the horizontal branch (HB), which is composed of two main groups of stars: the luminous blue HB stars, which extend by evolution into the RR Lyrae and red HB region, and a fainter, extremely blue population. We examine …

2011 Monthly Notices of the Royal Astronomical Society
eHST 60
Amplitude dependence of frequency sweep rates of whistler mode chorus emissions
DOI: 10.1029/2011JA016496 Bibcode: 2011JGRA..116.7201K

Katoh, Yuto; Omura, Yoshiharu

The frequency and amplitude characteristics of chorus emissions are studied by performing electron hybrid code simulations with different initial number densities of energetic electrons. Chorus emissions with rising tones are generated in all simulation runs except for the simulation assuming the lowest number density. The frequency sweep rates of…

2011 Journal of Geophysical Research (Space Physics)
Cluster 60
A large population of ultra-compact dwarf galaxies in the Hydra I cluster
DOI: 10.1051/0004-6361/201116728 Bibcode: 2011A&A...531A...4M

Hilker, M.; Georgiev, I. Y.; Richtler, T. +3 more


Aims: We performed a large spectroscopic survey of compact, unresolved objects in the core of the Hydra I galaxy cluster (Abell 1060), with the aim of identifying ultra-compact dwarf galaxies (UCDs) and investigating the properties of the globular cluster (GC) system around the central cD galaxy NGC 3311.
Methods: We obtained VIMOS mediu…

2011 Astronomy and Astrophysics
eHST 60
X-Ray Spectral Constraints for z ≈ 2 Massive Galaxies: The Identification of Reflection-dominated Active Galactic Nuclei
DOI: 10.1088/0004-637X/738/1/44 Bibcode: 2011ApJ...738...44A

Daddi, E.; Lehmer, B. D.; Alexander, D. M. +18 more

We use the 4 Ms Chandra Deep Field-South (CDF-S) survey to place direct constraints on the ubiquity of z ≈ 2 heavily obscured active galactic nuclei (AGNs) in K < 22 BzK-selected galaxies. Forty-seven (≈21%) of the 222 BzK-selected galaxies in the central region of the CDF-S are detected at X-ray energies, 11 (≈5%) of which have hard X-ray spec…

2011 The Astrophysical Journal
Suzaku 60
Average magnetotail electron and proton pitch angle distributions from Cluster PEACE and CIS observations
DOI: 10.1029/2011GL046770 Bibcode: 2011GeoRL..38.6103W

Dandouras, I.; Fazakerley, A. N.; Owen, C. J. +2 more

We present results from the first systematic survey of proton and electron pitch angle distributions in the magnetotail, based on Cluster CIS and PEACE data binned by proton plasma β (βp). The proton distributions conform to the canonical picture of magnetotail ions - a boundary layer made up of Earthward streaming and bidirectional fie…

2011 Geophysical Research Letters
Cluster 59
Mars ionosphere: A review of experimental results and modeling studies
DOI: 10.1029/2011RG000357 Bibcode: 2011RvGeo..49.4001H

Kallio, E.; Haider, S. A.; Mahajan, K. K.

In this paper we review results from atmospheric and ionospheric experiments on the early planetary missions like the Mariners, Mars, and Viking 1 and 2 Orbiters/Landers. We then discuss the new results obtained from the two latest missions, namely, the Mars Global Surveyor (MGS) and Mars Express (MEX). The MGS had three ionospheric and atmospheri…

2011 Reviews of Geophysics
MEx 59
Integral field spectroscopy of nitrogen overabundant blue compact dwarf galaxies
DOI: 10.1051/0004-6361/201116582 Bibcode: 2011A&A...532A.141P

Kehrig, C.; Pérez-Montero, E.; Vílchez, J. M. +6 more

Context. The oxygen and nitrogen-to-oxygen abundances relation is characterized by a plateau around log(N/O) = -1.6 at metallicities lower than 12+log(O/H) ~ 8.25. However, there is a subset of blue compact dwarf galaxies (BCDs) with unexpectedly high N/O values.
Aims: We want to study the spatial distribution of the physical properties and o…

2011 Astronomy and Astrophysics
eHST 59
XMM-Newton X-ray and Ultraviolet Observations of the Fast Nova V2491 Cyg during the Supersoft Source Phase
DOI: 10.1088/0004-637X/733/1/70 Bibcode: 2011ApJ...733...70N

Ness, J. -U.; Hernanz, M.; Sala, G. +12 more

Two XMM-Newton observations of the fast classical nova V2491 Cyg were carried out in short succession on days 39.93 and 49.62 after discovery, during the supersoft source (SSS) phase, yielding simultaneous X-ray and UV light curves and high-resolution X-ray spectra. The first X-ray light curve is highly variable, showing oscillations with a period…

2011 The Astrophysical Journal
XMM-Newton 59
Galactic cold cores. II. Herschel study of the extended dust emission around the first Planck detections
DOI: 10.1051/0004-6361/201015916 Bibcode: 2011A&A...527A.111J

Abergel, A.; Bernard, J. -P.; Dickinson, C. +15 more

Context. Within the project Galacticcoldcores we are carrying out Herschel photometric observations of cold interstellar clouds detected with the Planck satellite. The three fields observed as part of the Herschel science demonstration phase (SDP) provided the first glimpse into the nature of these sources. The aim of the project is to derive the …

2011 Astronomy and Astrophysics
Herschel Planck 59
X-Ray Spectroscopy of the High-mass X-Ray Binary Pulsar Centaurus X-3 over Its Binary Orbit
DOI: 10.1088/0004-637X/737/2/79 Bibcode: 2011ApJ...737...79N

Paul, Biswajit; Naik, Sachindra; Ali, Zulfikar

We present a comprehensive spectral analysis of the high-mass X-ray binary (HMXB) pulsar Centaurus X-3 with the Suzaku observatory covering nearly one orbital period. The light curve shows the presence of extended dips which are rarely seen in HMXBs. These dips are seen up to as high as ~40 keV. The pulsar spectra during the eclipse, out-of-eclips…

2011 The Astrophysical Journal
Suzaku 59