Search Publications

Ion Acceleration at the Earth's Bow Shock
DOI: 10.1007/s11214-012-9901-5 Bibcode: 2012SSRv..173....5B

Möbius, E.; Scholer, M.; Burgess, D.

The Earth's bow shock is the most studied example of a collisionless shock in the solar system. It is also widely used to model or predict the behaviour at other astrophysical shock systems. Spacecraft observations, theoretical modelling and numerical simulations have led to a detailed understanding of the bow shock structure, the spatial organiza…

2012 Space Science Reviews
Cluster 109
Quantitative Spectroscopy of Blue Supergiant Stars in the Disk of M81: Metallicity, Metallicity Gradient, and Distance
DOI: 10.1088/0004-637X/747/1/15 Bibcode: 2012ApJ...747...15K

Bresolin, Fabio; Kudritzki, Rolf-Peter; Urbaneja, Miguel A. +4 more

The quantitative spectral analysis of low-resolution (~5 Å) Keck LRIS spectra of blue supergiants in the disk of the giant spiral galaxy M81 is used to determine stellar effective temperatures, gravities, metallicities, luminosities, interstellar reddening, and a new distance using the flux-weighted gravity-luminosity relationship. Substantial red…

2012 The Astrophysical Journal
eHST 109
The Fermi GBM Gamma-Ray Burst Catalog: The First Two Years
DOI: 10.1088/0067-0049/199/1/18 Bibcode: 2012ApJS..199...18P

Goldstein, Adam; Preece, Robert D.; Kouveliotou, Chryssa +26 more

The Fermi Gamma-ray Burst Monitor (GBM) is designed to enhance the scientific return from Fermi in studying gamma-ray bursts (GRBs). In its first two years of operation GBM triggered on 491 GRBs. We summarize the criteria used for triggering and quantify the general characteristics of the triggered GRBs, including their locations, durations, peak …

2012 The Astrophysical Journal Supplement Series
INTEGRAL 109
The heating of dust by old stellar populations in the bulge of M31
DOI: 10.1111/j.1365-2966.2012.21696.x Bibcode: 2012MNRAS.426..892G

Schinnerer, Eva; Rix, Hans-Walter; Walter, Fabian +9 more

We use new Herschel multiband imaging of the Andromeda galaxy to analyse how dust heating occurs in the central regions of galaxy spheroids that are essentially devoid of young stars. We construct a dust temperature map of M31 through fitting modified blackbodies to the Herschel data, and find that the temperature within 2 kpc rises strongly from …

2012 Monthly Notices of the Royal Astronomical Society
Herschel 109
Herschel measurements of the D/H and 16O/18O ratios in water in the Oort-cloud comet C/2009 P1 (Garradd)
DOI: 10.1051/0004-6361/201219744 Bibcode: 2012A&A...544L..15B

Küppers, M.; Hartogh, P.; Lellouch, E. +19 more

The D/H ratio in cometary water is believed to be an important indicator of the conditions under which icy planetesimals formed and can provide clues to the contribution of comets to the delivery of water and other volatiles to Earth. Available measurements suggest that there is isotopic diversity in the comet population. The Herschel Space Observ…

2012 Astronomy and Astrophysics
Herschel 108
Auroral evidence of Io's control over the magnetosphere of Jupiter
DOI: 10.1029/2011GL050253 Bibcode: 2012GeoRL..39.1105B

Bonfond, B.; Clarke, J. T.; Gérard, J. -C. +5 more

Contrary to the case of the Earth, the main auroral oval on Jupiter is related to the breakdown of plasma corotation in the middle magnetosphere. Even if the root causes for the main auroral emissions are Io's volcanism and Jupiter's fast rotation, changes in the aurora could be attributed either to these internal factors or to fluctuations of the…

2012 Geophysical Research Letters
eHST 108
Inverse Compton X-Ray Emission from Supernovae with Compact Progenitors: Application to SN2011fe
DOI: 10.1088/0004-637X/751/2/134 Bibcode: 2012ApJ...751..134M

Hurley, K.; Costa, E.; Fransson, C. +39 more

We present a generalized analytic formalism for the inverse Compton X-ray emission from hydrogen-poor supernovae and apply this framework to SN 2011fe using Swift X-Ray Telescope (XRT), UVOT, and Chandra observations. We characterize the optical properties of SN 2011fe in the Swift bands and find them to be broadly consistent with a "normal" SN Ia…

2012 The Astrophysical Journal
INTEGRAL 108
Saturn's icy satellites and rings investigated by Cassini-VIMS: III - Radial compositional variability
DOI: 10.1016/j.icarus.2012.06.040 Bibcode: 2012Icar..220.1064F

Brown, R. H.; Baines, K. H.; Buratti, B. J. +16 more

In the last few years Cassini-VIMS, the Visible and Infrared Mapping Spectrometer, returned to us a comprehensive view of the Saturn's icy satellites and rings. After having analyzed the satellites' spectral properties (Filacchione, G., Capaccioni, F., McCord, T.B., Coradini, A., Cerroni, P., Bellucci, G., Tosi, F., D'Aversa, E., Formisano, V., Br…

2012 Icarus
Cassini 108
Hubble Space Telescope Hα imaging of star-forming galaxies at z ≃ 1-1.5: evolution in the size and luminosity of giant H II regions
DOI: 10.1111/j.1365-2966.2012.21900.x Bibcode: 2012MNRAS.427..688L

Rigby, J. R.; Smail, Ian; Jones, T. +10 more

We present Hubble Space Telescope/Wide Field Camera 3 narrow-band imaging of the Hα emission in a sample of eight gravitationally lensed galaxies at z = 1-1.5. The magnification caused by the foreground clusters enables us to obtain a median source plane spatial resolution of 360 pc, as well as providing magnifications in flux ranging from ∼10× to…

2012 Monthly Notices of the Royal Astronomical Society
eHST 108
What can We Learn about Solar Coronal Mass Ejections, Coronal Dimmings, and Extreme-ultraviolet Jets through Spectroscopic Observations?
DOI: 10.1088/0004-637X/748/2/106 Bibcode: 2012ApJ...748..106T

He, Jiansen; Wang, Xin; McIntosh, Scott W. +2 more

Solar eruptions, particularly coronal mass ejections (CMEs) and extreme-ultraviolet (EUV) jets, have rarely been investigated with spectroscopic observations. We analyze several data sets obtained by the EUV Imaging Spectrometer on board Hinode and find various types of flows during CMEs and jet eruptions. CME-induced dimming regions are found to …

2012 The Astrophysical Journal
Hinode 108