Search Publications

Sources of electron pitch angle anisotropy in the magnetotail plasma sheet
DOI: 10.1002/jgra.50553 Bibcode: 2013JGRA..118.6042W

Fazakerley, A. N.; Owen, C. J.; Taylor, M. G. G. T. +3 more

We survey the properties of electron pitch angle distributions in the magnetotail plasma sheet at a distance between 15 and 19 RE from the Earth, using data from the Plasma Electron and Current Experiment (PEACE) instrument. We limit our survey to those pitch angle distributions measured when the interplanetary magnetic field (IMF) had …

2013 Journal of Geophysical Research (Space Physics)
Cluster 33
Toward a Removal of Temperature Dependencies from Abundance Determinations: NGC 628
DOI: 10.1088/0004-637X/777/2/96 Bibcode: 2013ApJ...777...96C

Armus, L.; Hunt, L. K.; Pellegrini, E. +16 more

The metal content of a galaxy, a key property for distinguishing between viable galaxy evolutionary scenarios, strongly influences many of the physical processes in the interstellar medium. An absolute and robust determination of extragalactic metallicities is essential in constraining models of chemical enrichment and chemical evolution. Current …

2013 The Astrophysical Journal
Herschel 33
The High-ion Content and Kinematics of Low-redshift Lyman Limit Systems
DOI: 10.1088/0004-637X/778/2/187 Bibcode: 2013ApJ...778..187F

Tripp, Todd M.; Prochaska, J. Xavier; Davé, Romeel +9 more

We study the high-ion content and kinematics of the circumgalactic medium around low-redshift galaxies using a sample of 23 Lyman limit systems (LLSs) at 0.08 < z < 0.93 observed with the Cosmic Origins Spectrograph on board the Hubble Space Telescope. In Lehner et al., we recently showed that low-z LLSs have a bimodal metallicity distributi…

2013 The Astrophysical Journal
eHST 33
A Direct Stellar Metallicity Determination in the Disk of the Maser Galaxy NGC 4258
DOI: 10.1088/2041-8205/779/2/L20 Bibcode: 2013ApJ...779L..20K

Hosek, Matthew W., Jr.; Bresolin, Fabio; Kudritzki, Rolf-Peter +4 more

We present the first direct determination of a stellar metallicity in the spiral galaxy NGC 4258 (D = 7.6 Mpc) based on the quantitative analysis of a low-resolution (~5 Å) Keck Low Resolution Imaging Spectrograph spectrum of a blue supergiant star located in its disk. A determination of stellar metallicity in this galaxy is important for the abso…

2013 The Astrophysical Journal
eHST 32
The thermal dust emission in N158-N159-N160 (LMC) star-forming complex mapped by Spitzer, Herschel and LABOCA
DOI: 10.1093/mnras/stt280 Bibcode: 2013MNRAS.431.1596G

van Loon, J. Th.; Okumura, K.; Lebouteiller, V. +21 more

Low-metallicity galaxies exhibit different properties of the interstellar medium (ISM) compared to nearby spiral galaxies. Obtaining a resolved inventory of the various gas and dust components of massive star-forming regions and diffuse ISM is necessary to understand how those differences are driven. We present a study of the infrared/submillimetr…

2013 Monthly Notices of the Royal Astronomical Society
Herschel 32
On the nature of the hard X-ray sources SWIFT J1907.3-2050, IGR J12123-5802 and IGR J19552+0044
DOI: 10.1093/mnras/stt1434 Bibcode: 2013MNRAS.435.2822B

Mukai, K.; de Martino, D.; Masetti, N. +7 more

The INTEGRAL and Swift hard X-ray surveys have identified a large number of new sources, among which many are proposed as Cataclysmic Variables (CVs). Here, we present the first detailed study of three X-ray-selected CVs, Swift J1907.3-2050, IGR J12123-5802 and IGR J19552+0044 based on XMM-Newton, Suzaku, Swift observations and ground-based optica…

2013 Monthly Notices of the Royal Astronomical Society
INTEGRAL Suzaku XMM-Newton 32
The interaction-driven starburst contribution to the cosmic star formation rate density
DOI: 10.1051/0004-6361/201220754 Bibcode: 2013A&A...552A..44L

Fiore, F.; Santini, P.; Menci, N. +1 more

An increasing amount of observational evidence supports the notion that there are two modes of star formation: a quiescent mode in disk-like galaxies and a starburst mode, which is generally interpreted as driven by merging. Using a semi-analytic model of galaxy formation, we derive the relative contribution to the cosmic star formation rate densi…

2013 Astronomy and Astrophysics
Herschel 32
A Study of a Failed Coronal Mass Ejection Core Associated with an Asymmetric Filament Eruption
DOI: 10.1088/0004-637X/771/1/65 Bibcode: 2013ApJ...771...65J

Joshi, Navin Chandra; Filippov, Boris; Srivastava, Abhishek K. +3 more

We present multi-wavelength observations of an asymmetric filament eruption and associated coronal mass ejection (CME) and coronal downflows on 2012 June 17 and 18 from 20:00-05:00 UT. We use SDO/AIA and STEREO-B/SECCHI observations to understand the filament eruption scenario and its kinematics, while LASCO C2 observations are analyzed to study t…

2013 The Astrophysical Journal
SOHO 32
Discovering young stars in the Gum 31 region with infrared observations
DOI: 10.1051/0004-6361/201220218 Bibcode: 2013A&A...552A..14O

Grellmann, R.; Preibisch, T.; Roccatagliata, V. +4 more

Context. The Gum 31 bubble, which contains the stellar cluster NGC 3324, is a poorly studied young region close to the Carina Nebula.
Aims: We are aiming to characterise the young stellar and protostellar population in and around Gum 31 and to investigate the star-formation process in this region.
Methods: We identified candidate young s…

2013 Astronomy and Astrophysics
Herschel eHST 32
γ Doradus pulsation in two pre-main sequence stars discovered by CoRoT
DOI: 10.1051/0004-6361/201220127 Bibcode: 2013A&A...550A.121Z

Chaintreuil, S.; Ryabchikova, T.; Fossati, L. +5 more

Context. Pulsations in pre-main sequence stars have been discovered several times within the last years. But nearly all of these pulsators are of δ Scuti-type. γ Doradus-type pulsation in young stars has been predicted by theory, but lack observational evidence.
Aims: We present the investigation of variability caused by rotation and (γ Dorad…

2013 Astronomy and Astrophysics
CoRoT 32