Search Publications

Suzaku Monitoring of the Iron K Emission Line in the Type 1 Active Galactic Nucleus NGC 5548
DOI: 10.1088/0004-637X/710/2/1228 Bibcode: 2010ApJ...710.1228L

Elvis, Martin; Wilkes, Belinda J.; Nicastro, Fabrizio +10 more

We present seven sequential weekly observations of NGC 5548 conducted in 2007 with the Suzaku X-ray Imaging Spectrometer (XIS) in the 0.2-12 keV band and Hard X-ray Detector (HXD) in the 10-600 keV band. The iron Kα line is well detected in all seven observations and Kβ line is also detected in four observations. In this paper, we investigate the …

2010 The Astrophysical Journal
Suzaku 26
Long-term Multi-wavelength Studies of GRS 1915+105. I. A High-energy and Mid-infrared Focus with RXTE/INTEGRAL and Spitzer
DOI: 10.1088/0004-637X/715/2/1191 Bibcode: 2010ApJ...715.1191R

Chaty, S.; Rahoui, F.; Rodriguez, J. +3 more

To date, mid-infrared properties of Galactic black hole binaries have barely been investigated in the framework of multi-wavelength campaigns. Yet, studies in this spectral domain are crucial to get complementary information on the presence of dust and/or on the physical processes such as dust heating and thermal bremsstrahlung. Here, we report a …

2010 The Astrophysical Journal
INTEGRAL 26
Spectroscopy of M81 Globular Clusters
DOI: 10.1088/0004-6256/139/6/2620 Bibcode: 2010AJ....139.2620N

Nantais, Julie B.; Huchra, John P.

We obtained spectra of 74 globular clusters (GCs) in M81. These GCs had been identified as candidates in a Hubble Space Telescope (HST) Advanced Camera for Surveys I-band survey. Sixty-eight of these 74 clusters lie within 7' of the M81 nucleus. Sixty-two of these clusters are newly spectroscopically confirmed, more than doubling the number of con…

2010 The Astronomical Journal
eHST 26
Reversal of infall in SgrB2(M) revealed by Herschel/HIFI observations of HCN lines at THz frequencies
DOI: 10.1051/0004-6361/201015106 Bibcode: 2010A&A...521L..46R

Menten, K. M.; Martin, P. G.; Murphy, J. A. +54 more


Aims: To investigate the accretion and feedback processes in massive star formation, we analyze the shapes of emission lines from hot molecular cores, whose asymmetries trace infall and expansion motions.
Methods: The high-mass star forming region SgrB2(M) was observed with Herschel/HIFI (HEXOS key project) in various lines of HCN and it…

2010 Astronomy and Astrophysics
Herschel 26
Rift zone volcanism and associated cinder cone field in Utopia Planitia, Mars
DOI: 10.1029/2010JE003578 Bibcode: 2010JGRE..11512019L

Neukum, G.; Wagner, R.; Lanz, J. K. +2 more

We analyzed a small cone field in SW Utopia Planitia that shows striking similarities to volcanic rift zones on Earth. This is of particular interest as the study area lies off any of the volcanic centers of Mars in the northern hemisphere lowlands and is surrounded by material of the Amazonian aged Vastitas Borealis Formation (VBF). We believe th…

2010 Journal of Geophysical Research (Planets)
MEx 26
Coronal Mass Ejections and Sunspots—Solar Cycle Perspective
DOI: 10.1088/2041-8205/712/1/L77 Bibcode: 2010ApJ...712L..77R

Ramesh, K. B.

Recent studies have indicated that the occurrence of the maxima of coronal mass ejection (CME) rate and sunspot number (SSN) were nearly two years apart. We find that the two-year lag of CME rate manifests only when the SSN index is considered and the lag is minimal (two-three months) when the sunspot area is considered. CMEs with speeds greater t…

2010 The Astrophysical Journal
SOHO 26
Dune morphology, sand transport pathways and possible source areas in east Thaumasia Region (Mars)
DOI: 10.1016/j.geomorph.2009.07.019 Bibcode: 2010Geomo.121...84S

Silvestro, S.; Di Achille, G.; Ori, G. G.

An aeolian system located in Aonia Terra (eastern Thaumasia region) consists of six dark dune fields. The dune pattern suggests an organized extended sand transport system, which is characterized by the presence of long sand corridors. The latter connects the different ergs with potential sources. The sand stored in the ergs is provided by layered…

2010 Geomorphology
MEx 26
The radius and effective temperature of the binary Ap star β CrB from CHARA/FLUOR and VLT/NACO observations
DOI: 10.1051/0004-6361/200913405 Bibcode: 2010A&A...512A..55B

Kervella, P.; Kiss, L. L.; Tuthill, P. G. +14 more

Context. The prospects for using the asteroseismology of rapidly oscillating Ap (roAp) stars are hampered by the large uncertainty in fundamental stellar parameters. Results in the literature for the effective temperature (Teff) often span a range of 1000 K.
Aims: Our goal is to reduce systematic errors and improve the Teff

2010 Astronomy and Astrophysics
IUE 26
A Hemispheric Helicity Sign Rule Indicated by Large-scale Photospheric Magnetic Fields at Three Phases of Solar Cycle 23
DOI: 10.1088/0004-637X/720/1/632 Bibcode: 2010ApJ...720..632W

Zhang, Mei; Wang, Chuanyu

The hemispheric sign rule of current helicity is examined for large-scale magnetic fields, extending to 60° high in solar latitudes, at three different phases of solar cycle 23 and using three different instruments. The current helicity is calculated from the vector magnetic fields derived respectively from the longitudinal full-disk magnetograms …

2010 The Astrophysical Journal
SOHO 26
Far-infrared line imaging of the starburst ring in NGC 1097 with the Herschel/PACS spectrometer
DOI: 10.1051/0004-6361/201014592 Bibcode: 2010A&A...518L..60B

Helou, G.; Roussel, H.; Murphy, E. J. +38 more

NGC 1097 is a nearby SBb galaxy with a Seyfert nucleus and a bright starburst ring. We study the physical properties of the interstellar medium (ISM) in the ring using spatially resolved far-infrared spectral maps of the circumnuclear starburst ring of NGC 1097, obtained with the PACS spectrometer on board the Herschel Space Observatory. In partic…

2010 Astronomy and Astrophysics
Herschel 26