Search Publications

On the combination of ACE data with numerical simulations to determine the initial characteristics of a CME
DOI: 10.1051/0004-6361:200811022 Bibcode: 2008A&A...492L..29C

Poedts, S.; Chané, E.; van der Holst, B.

Aims: Our goal is to combine the Advanced Composition Explorer (ACE) data with numerical simulations to determine the initial characteristics of the halo coronal mass ejection (CME), which was observed on April 4, 2000.
Methods: The evolution of a CME from the Sun to 1 AU is simulated in the framework of 2.5 D (axi-symmetric) ideal Magnetohydr…

2008 Astronomy and Astrophysics
SOHO 23
PKS2250-41: a case study for triggering
DOI: 10.1111/j.1365-2966.2008.13171.x Bibcode: 2008MNRAS.386.1797I

Villar-Martín, M.; Morganti, R.; Tadhunter, C. N. +3 more

We present the results of a multiwavelength study of the z = 0.31 radio source PKS2250-41. Integral field unit and long-slit spectroscopy obtained using VIMOS and FORS1 on the VLT, and archival Hubble Space Telescope optical imaging observations are used to study the morphology, kinematics and ionization state of the extended emission-line region …

2008 Monthly Notices of the Royal Astronomical Society
eHST 23
X-Ray Observations of the Coma Cluster in a Broad Energy Band with the INTEGRAL, RXTE, and ROSAT Observatories
DOI: 10.1086/592032 Bibcode: 2008ApJ...687..968L

Sunyaev, R. A.; Vikhlinin, A.; Lutovinov, A. A. +2 more

We present results of X-ray observations of the Coma Cluster with multiple instruments over a broad energy band. Using the data from the INTEGRAL, RXTE, and ROSAT observatories, we find that the Coma spectrum in the 0.5-107 keV energy band can be well approximated by a thermal plasma emission model with a temperature of T = 8.2 keV. INTEGRAL was u…

2008 The Astrophysical Journal
INTEGRAL 23
Intensity oscillations and heating of the coronal X-ray bright points from Hinode/XRT
DOI: 10.1051/0004-6361:20079127 Bibcode: 2008A&A...485..289K

Kariyappa, R.; Varghese, B. A.

Aims: Our aim is to investigate the intensity oscillations in coronal X-ray Bright Points (XBPs).
Methods: We analysed a 7 h long time sequence of the soft X-ray images obtained on April 14, 2007 with a 2 min cadence using the X-Ray Telescope (XRT) on-board the Hinode mission. We use SSW in IDL to derive the time series of 14 XBPs and 2 backgr…

2008 Astronomy and Astrophysics
Hinode 23
Preliminary orbital elements of six visual binary stars
DOI: 10.1002/asna.200710966 Bibcode: 2008AN....329..379S

Scardia, M.; Prieur, J. -L.; Pansecchi, L. +1 more

Preliminary new orbital elements were computed for the visual binary stars A 1 - ADS 1345, A 2629 - ADS 3610, BU 560 - ADS 4371, STF 3115 - ADS 4376, STF 1426 AB - ADS 7730 and STF 2437 - ADS 11956. Using Straizys and Kuriliene's data, we derived new formulae for computing dynamical parallaxes for luminosity classes IV and V. The values found for …

2008 Astronomische Nachrichten
Hipparcos 23
The Evolution of Late-Time Optical Emission from SN 1986J
DOI: 10.1086/590426 Bibcode: 2008ApJ...684.1170M

Kirshner, Robert P.; Leibundgut, Bruno; Milisavljevic, Dan +1 more

We present late-time optical images and spectra of the Type IIn supernova SN 1986J. HST ACS/WFC images obtained in 2003 February show it to be still relatively bright, with mF606W = 21.4 and mF814W = 20.0 mag. Compared to 1994 December HST WFPC2 images, SN 1986J shows a decline of only lesssim1 mag in brightness over 8 years.…

2008 The Astrophysical Journal
eHST 23
Magnetic complexity in eruptive solar active regions and associated eruption parameters
DOI: 10.1029/2007GL032040 Bibcode: 2008GeoRL..35.6S02G

Georgoulis, Manolis K.

Using an efficient magnetic complexity index in the active-region solar photosphere, we quantify the preflare strength of the photospheric magnetic polarity inversion lines in 23 eruptive active regions with flare/CME/ICME events tracked all the way from the Sun to the Earth. We find that active regions with more intense polarity inversion lines h…

2008 Geophysical Research Letters
SOHO 23
Solar Radio Spikes in 2.6 - 3.8 GHz during the 13 December 2006 Event
DOI: 10.1007/s11207-008-9278-5 Bibcode: 2008SoPh..253..133W

Zhang, Y.; Yan, Y. H.; Liu, Y. Y. +3 more

On 13 December 2006, some unusual radio bursts in the range 2.6 - 3.8 GHz were observed during an X3.4 flare/CME event from 02:30 to 04:30 UT in active region NOAA 10930 (S06W27) with the digital spectrometers of the National Astronomical Observatories of China (NAOC). During this event many spikes were detected with the high temporal resolution o…

2008 Solar Physics
Hinode 23
The EBIT Calorimeter Spectrometer: A New, Permanent User Facility at the LLNL EBIT
DOI: 10.1007/s10909-008-9788-4 Bibcode: 2008JLTP..151.1061P

Kilbourne, C. A.; Porter, F. S.; Kelley, R. L. +8 more

The EBIT Calorimeter Spectrometer (ECS) is currently being completed and will be installed at the EBIT facility at the Lawrence Livermore National Laboratory in October 2007. The ECS will replace the smaller XRS/EBIT microcalorimeter spectrometer that has been in almost continuous operation since 2000. The XRS/EBIT was based on a spare laboratory …

2008 Journal of Low Temperature Physics
Suzaku 23
Gemini Spectroscopy and HST Imaging of the Stellar Cluster Population in Region B of M82
DOI: 10.1086/524133 Bibcode: 2008ApJ...674..846K

Bastian, N.; Smith, L. J.; Gallagher, J. S., III +3 more

We present new spectroscopic observations of the stellar cluster population of region B in the prototype starburst galaxy M82 obtained with the Gemini North 8.1 m telescope. By coupling the spectroscopy with UBVI photometry acquired with the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope (HST), we derive ages, extinctions, and rad…

2008 The Astrophysical Journal
eHST 23