Search Publications

Local influence of magnetosheath plasma beta fluctuations on magnetopause reconnection
DOI: 10.5194/angeo-28-1053-2010 Bibcode: 2010AnGeo..28.1053L

André, M.; Vaivads, A.; Rème, H. +2 more

We present observations from two subsolar Cluster magnetopause crossings under southward interplanetary magnetic field and strong mirror mode fluctuations in the magnetosheath. In both events the reconnection outflow jets show strong variations on the timescale of one minute. We show that at least some of the recorded variations are truly temporal…

2010 Annales Geophysicae
Cluster 10
Lithium Abundance in Solar-type Stars with Low Chromospheric Activity: Application to the Search for Maunder Minimum Analogs
DOI: 10.1088/0004-637X/716/1/766 Bibcode: 2010ApJ...716..766L

Tytler, David; Lubin, Dan; Kirkman, David

We use measurements of lithium abundance to examine the evolutionary history of stars frequently believed to be in a Maunder minimum (MM) state due to their low chromospheric activity. In a sample whose main-sequence membership has been verified using Hipparcos parallax data, we find that stars with very low chromospheric activity log R'HK

2010 The Astrophysical Journal
Hipparcos 10
Cold dust clumps in dynamically hot gas
DOI: 10.1051/0004-6361/201014645 Bibcode: 2010A&A...518L..75K

Poglitsch, A.; Bernard, J. -P.; Reach, W. T. +27 more


Aims: We present clumps of dust emission from Herschel observations of the Large Magellanic Cloud (LMC) and their physical and statistical properties. We catalog cloud features seen in the dust emission from Herschel observations of the LMC, the Magellanic type irregular galaxy closest to the Milky Way, and compare these features with H i cat…

2010 Astronomy and Astrophysics
Herschel 10
The Type Ib supernova 2010O: an explosion in a Wolf-Rayet X-ray binary?
DOI: 10.1111/j.1745-3933.2010.00861.x Bibcode: 2010MNRAS.405L..71N

Nelemans, Gijs; Voss, Rasmus; Nielsen, Mikkel T. B. +1 more

The Type Ib supernova 2010O was recently discovered in the interacting starburst galaxy Arp 299. We present an analysis of two archival Chandra X-ray observations of Arp 299 taken before the explosion and show that there is a transient X-ray source at a position consistent with the supernova. Due to the diffuse emission, the background is difficul…

2010 Monthly Notices of the Royal Astronomical Society
eHST 10
V5116 Sgr: A disc-eclipsed SSS post-outburst nova?
DOI: 10.1002/asna.200911327 Bibcode: 2010AN....331..201S

Greiner, J.; Hernanz, M.; Sala, G. +1 more

Nova V5116 Sgr 2005 No. 2, discovered on 2005 July 4, was observed with XMM-Newton in March 2007, 20 months after the optical outburst. The X-ray spectrum showed that the nova had evolved to a pure supersoft X-ray source, indicative of residual H-burning on top of the white dwarf. The X-ray light-curve shows abrupt decreases and increases of the f…

2010 Astronomische Nachrichten
XMM-Newton 10
New intrinsic-colour calibration for uvby- β photometry
DOI: 10.1016/j.newast.2009.12.003 Bibcode: 2010NewA...15..444K

Karataş, Yüksel; Schuster, William J.

A new intrinsic-colour calibration ((b-y)o-β) is presented for the uvby- β photometric system, making use of re-calibrated Hipparcos parallaxes and published reddening maps. This new calibration for (b-y)o-β, our Eq. (1), has been based upon stars with dHip<70pc in the photometric catalogues of Schuster and Niss…

2010 New Astronomy
Hipparcos 10
EC 11481–2303—a peculiar subdwarf OB star revisited
DOI: 10.1007/s10509-010-0304-3 Bibcode: 2010Ap&SS.329..133R

Rauch, Thomas; Werner, Klaus; Kruk, Jeffrey W.

EC 11481–2303 is a peculiar, hot, high-gravity pre-white dwarf. Previous optical spectroscopy revealed that it is a sdOB star with Teff=41 790 K, log g=5.84, and He/H = 0.014 by number. We present an on-going spectral analysis by means of non-LTE model-atmosphere techniques based on high-resolution, high-S/N optical (VLT-UVES) and ultra…

2010 Astrophysics and Space Science
IUE 10
When galaxies collide: understanding the broad absorption-line radio galaxy 4C +72.26
DOI: 10.1111/j.1365-2966.2010.16279.x Bibcode: 2010MNRAS.404.1089S

Jarvis, M. J.; Swinbank, A. M.; Rawlings, S. +2 more

We present a range of new observations of the `broad absorption-line radio galaxy' 4C +72.26 (z ~ 3.5), including sensitive rest-frame ultraviolet integral field spectroscopy using the Gemini/GMOS-N instrument and Subaru/CISCO K-band imaging and spectroscopy. We show that 4C +72.26 is a system of two vigorously star-forming galaxies superimposed a…

2010 Monthly Notices of the Royal Astronomical Society
eHST 10
The Extended X-ray Nebula of PSR J1420-6048
DOI: 10.1088/0004-637X/711/2/1168 Bibcode: 2010ApJ...711.1168V

Romani, Roger W.; Van Etten, Adam

The vicinity of the unidentified EGRET source 3EG J1420-6038 has undergone extensive study in the search for counterparts, revealing the energetic young pulsar PSR J1420-6048 and its surrounding wind nebula as a likely candidate for at least part of the emission from this bright and extended gamma-ray source. We report on new Suzaku observations o…

2010 The Astrophysical Journal
Suzaku XMM-Newton 10
The Galaxy Alignment Effect in Abell 1689: Evolution, Radial, and Luminosity Dependence
DOI: 10.1088/0004-637X/720/2/1483 Bibcode: 2010ApJ...720.1483H

De Propris, Roberto; Bañados, Eduardo; West, Michael J. +1 more

We measure alignments on scales of 1 Mpc h -1 71 for galaxies in Abell 1689 (z = 0.18) from an existing Hubble Space Telescope mosaic. We find evidence of galaxy alignment in the inner 500 h -1 71 kpc. The alignment appears to be stronger toward the center and is mostly present among the fainter galaxies…

2010 The Astrophysical Journal
eHST 10