Search Publications

Multi-wavelength observations and modelling of a canonical solar flare
DOI: 10.1051/0004-6361:200810437 Bibcode: 2009A&A...494.1127R

Klimchuk, J. A.; Gallagher, P. T.; Milligan, R. O. +1 more

Aims: We investigate the temporal evolution of temperature, emission measure, energy loss, and velocity in a C-class solar flare from both observational and theoretical perspectives.
Methods: The properties of the flare were derived by following the systematic cooling of the plasma through the response functions of a number of instruments - th…

2009 Astronomy and Astrophysics
SOHO 59
The Three-Dimensional Dynamic Structure of the Inner Orion Nebula
DOI: 10.1088/0004-6256/137/1/367 Bibcode: 2009AJ....137..367O

Abel, N. P.; O'Dell, C. R.; Henney, W. J. +2 more

The three-dimensional structure of the brightest part of the Orion Nebula is assessed in the light of published and newly established data. We find that the widely accepted model of a concave blister of ionized material needs to be altered in the southwest direction from the Trapezium, where we find that the Orion-S feature is a separate cloud of …

2009 The Astronomical Journal
eHST 59
High-energy characteristics of the schizophrenic pulsar PSR J1846-0258 in Kes 75. Multi-year RXTE and INTEGRAL observations crossing the magnetar-like outburst
DOI: 10.1051/0004-6361/200811580 Bibcode: 2009A&A...501.1031K

Kuiper, L.; Hermsen, W.

Aims: PSR J1846-0258 is a young rotation-powered pulsar with one of the highest surface magnetic field strengths, located in the centre of SN-remnant Kes-75. In June 2006 a magnetar-like outburst took place. Using multi-year RXTE and INTEGRAL observations covering the epoch of the outburst, we aim to study the temporal and spectral characteristics…

2009 Astronomy and Astrophysics
INTEGRAL 59
The X-ray view of giga-hertz peaked spectrum radio galaxies
DOI: 10.1051/0004-6361/200811284 Bibcode: 2009A&A...501...89T

Guainazzi, M.; Piconcelli, E.; Grandi, P. +5 more

Context: This paper presents the X-ray properties of a flux- and volume-limited complete sample of 16 giga-hertz peaked spectrum (GPS) galaxies.
Aims: This study addresses three basic questions in our understanding of the nature and evolution of GPS sources: a) What is the physical origin of the X-ray emission in GPS galaxies? b) Which physica…

2009 Astronomy and Astrophysics
XMM-Newton 59
The NGC 300 Transient: An Alternative Method for Measuring Progenitor Masses
DOI: 10.1088/0004-637X/703/1/300 Bibcode: 2009ApJ...703..300G

Williams, Benjamin F.; Dolphin, Andrew; Dalcanton, Julianne J. +3 more

We present an alternative technique for measuring the precursor masses of transient events in stars undergoing late stage stellar evolution. We use the well-established techniques of stellar population modeling to age-date the stars surrounding the site of the recent transient event in NGC 300 (NGC 300 OT2008-1). The surrounding stars must share a…

2009 The Astrophysical Journal
eHST 59
Correlated X-Ray and Very High Energy Emission in the Gamma-Ray Binary LS I +61 303
DOI: 10.1088/0004-637X/706/1/L27 Bibcode: 2009ApJ...706L..27A

Maraschi, L.; Covino, S.; Antonelli, L. A. +153 more

The discovery of very high energy (VHE) gamma-ray emitting X-ray binaries has triggered an intense effort to better understand the particle acceleration, absorption, and emission mechanisms in compact binary systems, which provide variable conditions along eccentric orbits. Despite this, the nature of some of these systems, and of the accelerated …

2009 The Astrophysical Journal
XMM-Newton 59
Some Like It Hot: Coronal Heating Observations from Hinode X-ray Telescope and RHESSI
DOI: 10.1088/0004-637X/704/1/863 Bibcode: 2009ApJ...704..863S

Lin, L.; Golub, L.; Schmelz, J. T. +7 more

We have used Hinode X-Ray Telescope observations and RHESSI upper limits together to characterize the differential emission measure (DEM) from a quiescent active region. We find a relatively smooth DEM curve with the expected active region peak at log T = 6.4. We also find a high-temperature component with significant emission measure at log T gsi…

2009 The Astrophysical Journal
Hinode 59
The velocity field of sunspot penumbrae. I. A global view
DOI: 10.1051/0004-6361/200913074 Bibcode: 2009A&A...508.1453F

Franz, M.; Schlichenmaier, R.

Aims. We investigated the vertical penumbral plasma flow on small spatial scales using data recorded by the spectropolarimeter of the solar optical telescope onboard Hinode.
Methods: We computed maps of apparent Doppler velocities by comparing the spectral positions of the Fe I 630.15 nm & Fe I 630.25 nm lines with the averaged line profil…

2009 Astronomy and Astrophysics
Hinode 59
New Observation of Failed Filament Eruptions: The Influence of Asymmetric Coronal Background Fields on Solar Eruptions
DOI: 10.1088/0004-637X/696/1/L70 Bibcode: 2009ApJ...696L..70L

Liu, Y.; Shibata, K.; Lin, H. +3 more

Failed filament eruptions not associated with a coronal mass ejection (CME) have been observed and reported as evidence for solar coronal field confinement on erupting flux ropes. In those events, each filament eventually returns to its origin on the solar surface. In this Letter, a new observation of two failed filament eruptions is reported whic…

2009 The Astrophysical Journal
SOHO 59
Possible pingo fields in the Utopia basin, Mars: Geological and climatical implications
DOI: 10.1016/j.icarus.2008.09.007 Bibcode: 2009Icar..199...49D

de Pablo, Miguel Ángel; Komatsu, Goro

The presence of pingos on Mars has been hypothesized since the period of the Viking mission. In fact, a diverse range of pingo-like features has been found at various martian sites including Elysium, Chryse and Utopia Planitiae in the northern lowlands. Due to the morphology and the geological setting, some of those features were interpreted in di…

2009 Icarus
MEx 59