Search Publications

A 205 µm [N II] Map of the Carina Nebula
DOI: 10.1088/0004-637X/739/2/100 Bibcode: 2011ApJ...739..100O

Stark, A. A.; Stacey, G. J.; Kamenetzky, J. +5 more

We present the results of a ~250 arcmin2 mapping of the 205 µm [N II] fine-structure emission over the northern Carina Nebula, including the Car I and Car II H II regions. Spectra were obtained using the South Pole Imaging Fabry-Perot Interferometer (SPIFI) at the Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) a…

2011 The Astrophysical Journal
ISO 53
A Correlation Between Host Star Activity and Planet Mass for Close-in Extrasolar Planets?
DOI: 10.1088/0004-637X/735/1/59 Bibcode: 2011ApJ...735...59P

Schmitt, J. H. M. M.; Poppenhaeger, K.

The activity levels of stars are influenced by several stellar properties, such as stellar rotation, spectral type, and the presence of stellar companions. Analogous to binaries, planetary companions are also thought to be able to cause higher activity levels in their host stars, although at lower levels. Especially in X-rays, such influences are …

2011 The Astrophysical Journal
XMM-Newton 53
Ensemble X-ray variability of active galactic nuclei from serendipitous source catalogues
DOI: 10.1051/0004-6361/201118072 Bibcode: 2011A&A...536A..84V

Trevese, D.; Vagnetti, F.; Turriziani, S.

Context. The X-ray variability of the active galactic nuclei (AGN) has been most often investigated with studies of individual, nearby sources, and only a few ensemble analyses have been applied to large samples in wide ranges of luminosity and redshift.
Aims: We aim to determine the ensemble variability properties of two serendipitously sele…

2011 Astronomy and Astrophysics
XMM-Newton 53
The star formation history in the far outer disc of M33
DOI: 10.1111/j.1365-2966.2010.17458.x Bibcode: 2011MNRAS.410..504B

Cole, A. A.; Tanvir, N. R.; Ferguson, A. M. N. +5 more

The outer regions of disc galaxies are becoming increasingly recognized as key testing sites for models of disc assembly and evolution. Important issues are the epoch at which the bulk of the stars in these regions formed and how discs grow radially over time. To address these issues, we use Hubble Space Telescope Advanced Camera for Surveys imagi…

2011 Monthly Notices of the Royal Astronomical Society
eHST 53
Bipolar electric field signatures of reconnection separatrices for a hydrogen plasma at realistic guide fields
DOI: 10.1029/2011GL048572 Bibcode: 2011GeoRL..3817104L

Divin, A.; Goldman, M. V.; Newman, D. L. +2 more

In preparation for the MMS mission we ask the question: how common are bipolar signatures linked to the presence of electron holes along separatrices emanating from reconnection regions? To answer this question, we conduct massively parallel simulations for realistic conditions and for the hydrogen mass ratio in boxes larger than considered in sim…

2011 Geophysical Research Letters
Cluster 53
Influence of negatively charged plume grains and hemisphere coupling currents on the structure of Enceladus' Alfvén wings: Analytical modeling of Cassini magnetometer observations
DOI: 10.1029/2010JA016338 Bibcode: 2011JGRA..116.4221S

Dougherty, Michele K.; Saur, Joachim; Kriegel, Hendrik +3 more

We present an analytical model of the Alfvén wing system that is generated by the interaction between the plume of Enceladus and the corotating plasma in Saturn's inner magnetosphere. Our primary purpose is to explain the orientation of the magnetic field perturbations detected in Enceladus' Alfvén wings by the Cassini magnetometer (MAG) instrumen…

2011 Journal of Geophysical Research (Space Physics)
Cassini 53
New insight into the formation of hexamethylenetetramine (HMT) in interstellar and cometary ice analogs
DOI: 10.1051/0004-6361/201116688 Bibcode: 2011A&A...530A.128V

Vinogradoff, V.; Duvernay, F.; Danger, G. +2 more


Aims: We investigate the purely thermal formation of hexamethylenetetramine (HMT, C6H12N4) in interstellar ice analogs from non-photolysed ice and compare our results with those for the formation from photolysed ice.
Methods: We use Fourier transform-infrared spectroscopy to follow residue formation from …

2011 Astronomy and Astrophysics
Rosetta 53
The Circumstellar Environment of R Coronae Borealis: White Dwarf Merger or Final-helium-shell Flash?
DOI: 10.1088/0004-637X/743/1/44 Bibcode: 2011ApJ...743...44C

Ivison, R. J.; Olofsson, G.; Bond, Howard E. +21 more

In 2007, R Coronae Borealis (R CrB) went into a historically deep and long decline. In this state, the dust acts like a natural coronagraph at visible wavelengths, allowing faint nebulosity around the star to be seen. Imaging has been obtained from 0.5 to 500 µm with Gemini/GMOS, Hubble Space Telescope/WFPC2, Spitzer/MIPS, and Herschel/SPIRE…

2011 The Astrophysical Journal
AKARI Herschel eHST 53
The Gradients in the 47 Tuc Red Giant Branch Bump and Horizontal Branch are Consistent with a Centrally Concentrated, Helium-enriched Second Stellar Generation
DOI: 10.1088/0004-637X/736/2/94 Bibcode: 2011ApJ...736...94N

Nataf, D. M.; Gould, A.; Pinsonneault, M. H. +1 more

We combine ground- and space-based photometry of the Galactic globular cluster 47 Tuc to measure four independent lines of evidence for a helium gradient in the cluster, whereby stars in the cluster outskirts would have a lower initial helium abundance than stars in and near the cluster core. For our first and second lines of evidence, we show tha…

2011 The Astrophysical Journal
eHST 53
X-ray reverberation close to the black hole in RE J1034+396
DOI: 10.1111/j.1365-2966.2011.19655.x Bibcode: 2011MNRAS.418.2642Z

Fabian, A. C.; Zoghbi, A.

In previous work, we discussed the detection of reverberation delays in the narrow-line Seyfert 1 (NLS1) 1H0707-495. The delays originate close to the black hole. Here, we show that RE J1034+396 shows very similar lag properties. At low frequencies (<1 × 10-4 Hz), the time lag between energy bands increases with energy separation, si…

2011 Monthly Notices of the Royal Astronomical Society
XMM-Newton 53