Search Publications

Effective area calibration of the reflection grating spectrometers of XMM-Newton. I. X-ray spectroscopy of the Crab nebula
DOI: 10.1051/0004-6361/20077892 Bibcode: 2009A&A...497..291K

Kaastra, J. S.; Costantini, E.; de Vries, C. P. +1 more

Context: The Crab nebula and pulsar have been widely used as a calibration source for X-ray instruments. The in-flight effective area calibration of the Reflection Grating Spectrometers (RGS) of XMM-Newton depend upon the availability of reliable calibration sources.
Aims: We investigate how the absolute effective area calibration of RGS can b…

2009 Astronomy and Astrophysics
XMM-Newton 36
3D Evolution of a Filament Disappearance Event Observed by STEREO
DOI: 10.1007/s11207-009-9448-0 Bibcode: 2009SoPh..259...13G

Schmieder, B.; Chandra, R.; Venkatakrishnan, P. +2 more

A filament disappearance event was observed on 22 May 2008 during our recent campaign JOP 178. The filament, situated in the Southern Hemisphere, showed sinistral chirality consistent with the hemispheric rule. The event was well observed by several observatories, in particular by THEMIS. One day, before the disappearance, Hα observations showed u…

2009 Solar Physics
SOHO 36
Hierarchical star formation: stars and stellar clusters in the Gould Belt
DOI: 10.1111/j.1365-2966.2009.14465.x Bibcode: 2009MNRAS.397....2E

Alfaro, E. J.; Cabrera-Caño, J.; Elias, F.

We perform a study of the spatial and kinematical distribution of young open clusters in the solar neighbourhood, discerning between bound clusters and transient stellar condensations within our sample. Then, we discriminate between Gould Belt (GB) and local Galactic disc (LGD) members, using our previous estimate of the structural parameters of b…

2009 Monthly Notices of the Royal Astronomical Society
Hipparcos 36
The EROS2 search for microlensing events towards the spiral arms: the complete seven season results
DOI: 10.1051/0004-6361/200811515 Bibcode: 2009A&A...500.1027R

Couchot, F.; Perdereau, O.; Andersen, J. +37 more

Aims: The EROS-2 project has been designed to search for microlensing events towards any dense stellar field. The densest parts of the Galactic spiral arms have been monitored to maximize the microlensing signal expected from the stars of the Galactic disk and bulge.
Methods: 12.9 million stars have been monitored during 7 seasons towards 4 di…

2009 Astronomy and Astrophysics
eHST 36
The Relationship between Coronal Dimming and Coronal Mass Ejection Properties
DOI: 10.1088/0004-637X/705/1/914 Bibcode: 2009ApJ...705..914R

Biesecker, D. A.; Reinard, A. A.

Coronal dimmings are closely related to the footpoints of coronal mass ejections (CMEs) and, as such, offer information about CME origins and evolution. In this paper, we investigate the relationship between CME and dimming properties. In particular, we compare CME quantities for events with and without associated dimmings. We find that dimming-as…

2009 The Astrophysical Journal
SOHO 36
The low-mass initial mass function in the young cluster NGC6611
DOI: 10.1111/j.1365-2966.2008.14140.x Bibcode: 2009MNRAS.392.1034O

van Loon, J. Th.; Jeffries, R. D.; Oliveira, J. M.

NGC6611 is the massive young cluster (2-3Myr) that ionizes the Eagle Nebula. We present very deep photometric observations of the central region of NGC6611 obtained with the Hubble Space Telescope and the following filters: ACS/WFC F775W and F850LP and NIC2 F110W and F160W, loosely equivalent to ground-based IZJH filters. This survey reaches down …

2009 Monthly Notices of the Royal Astronomical Society
eHST 36
Time-dependent global MHD simulations of Cassini T32 flyby: From magnetosphere to magnetosheath
DOI: 10.1029/2008JA013676 Bibcode: 2009JGRA..114.3204M

Coates, A. J.; Russell, C. T.; Dougherty, M. K. +10 more

When the Cassini spacecraft flew by Titan on 13 June 2007, at 13.6 Saturn local time, Titan was directly observed to be outside Saturn's magnetopause. Cassini observations showed dramatic changes of magnetic field orientation as well as other plasma flow parameters during the inbound and outbound segments. In this paper, we study Titan's ionospher…

2009 Journal of Geophysical Research (Space Physics)
Cassini 36
Reliability of prediction of the magnetosheath BZ component from interplanetary magnetic field observations
DOI: 10.1029/2009JA014552 Bibcode: 2009JGRA..11412213S

Němeček, Z.; Gutynska, O.; Šafránková, J. +2 more

In the present statistical study, we discuss a probability of simultaneous observations of the same sign of the magnetic field BZ component in the solar wind and magnetosheath. The analysis is based on 5 min data from four spacecraft (Interball-1, IMP 8, Cluster, and THEMIS) operating in different phases of the solar cycle in the magnet…

2009 Journal of Geophysical Research (Space Physics)
Cluster 36
Deep Chandra Monitoring Observations of NGC 4278: Catalog of Source Properties
DOI: 10.1088/0067-0049/181/2/605 Bibcode: 2009ApJS..181..605B

Zezas, A.; Gallagher, J.; King, A. R. +11 more

We present the properties of the discrete X-ray sources detected in our monitoring program of the globular cluster (GC) rich elliptical galaxy, NGC 4278, observed with Chandra ACIS-S in six separate pointings, resulting in a co-added exposure of 458 ks. From this deep observation, 236 sources have been detected within the region overlapped by all …

2009 The Astrophysical Journal Supplement Series
eHST 36
Suzaku and Multi-Wavelength Observations of OJ 287 during the Periodic Optical Outburst in 2007
DOI: 10.1093/pasj/61.5.1011 Bibcode: 2009PASJ...61.1011S

Isobe, Naoki; Kohno, Kotaro; Shimajiri, Yoshito +153 more

Suzaku observations of the blazar OJ 287 were performed in 2007 April 10-13 and November 7-9. They correspond to a quiescent and a flaring state, respectively. The X-ray spectra of the source can be well-described with single power-law models in both exposures. The derived X-ray photon index and the flux density at 1 keV were found to be Γ = 1.65±…

2009 Publications of the Astronomical Society of Japan
Suzaku 36