Search Publications

Search for Sc-K Line Emission from RX J0852.0-4622 Supernova Remnant with Suzaku
DOI: 10.1093/pasj/61.2.275 Bibcode: 2009PASJ...61..275H

Petre, Robert; Terada, Yukikatsu; Bamba, Aya +6 more

We searched for evidence of line emission around 4keV from the northwestern rim of the supernova remnant RX J0852.0-4622 using Suzaku XIS data. Several papers have reported on the detection of an emission line around 4.1keV from this region of the sky. This line would arise from K-band fluorescence by 44Sc, the immediate decay product o…

2009 Publications of the Astronomical Society of Japan
Suzaku 13
The 3D velocity structure of the planetary nebula NGC 7009
DOI: 10.48550/arXiv.0905.2148 Bibcode: 2009RMxAA..45..143S

Steffen, W.; Koning, N.; Espíndola, M. +1 more

In search for deviations from homologous expansion in planetary nebulae we present a 3D morphokinematical model of NGC 7009. The model has been constructed with Shape based on PV diagrams from the literature and HST images. We find that the data are consistent with a radial velocity field with increased gradient at high latitudes compared to the e…

2009 Revista Mexicana de Astronomia y Astrofisica
eHST 13
Magnetic evolution of superactive regions. Complexity and potentially unstable magnetic discontinuities
DOI: 10.1051/0004-6361/200912044 Bibcode: 2009A&A...506.1429C

Romano, P.; Zuccarello, F.; Giorgi, F. +1 more

Context: It is widely accepted that solar flares are manifestations of magnetic reconnection events taking place in the solar atmosphere. Several aspects of these events remain unclear, although many efforts have been devoted to the investigation of magnetic field configurations at flare occurrence sites.
Aims: In this work, we have studied th…

2009 Astronomy and Astrophysics
SOHO 13
Super Star Clusters in SBS0335-052E
DOI: 10.1088/0004-637X/691/2/1068 Bibcode: 2009ApJ...691.1068T

Schneider, Glenn; Kennicutt, Robert C.; Vanzi, Leonardo +3 more

As one of the lowest metallicity star-forming galaxies, with a nucleus of several super star clusters (SSCs), SBS0335-052E is the subject of substantial current study. We present new insights on this galaxy based on new and archival high spatial resolution NICMOS and attitude control system images. We provide new measurements and limits on the siz…

2009 The Astrophysical Journal
eHST 13
Titan at 3 microns: Newly identified spectral features and an improved analysis of haze opacity
DOI: 10.1016/j.icarus.2008.09.017 Bibcode: 2009Icar..199..449S

Kim, Sang Joon; Geballe, Thomas R.; Courtin, Régis +3 more

We have reanalyzed the high-resolution spectrum of Titan between 2.87 and 3.12 µm observed with NIRSPEC/Keck II on 2001 Nov. 21 in southern summer, using updated CH 3D and C 2H 6 line-by-line models. From new synthetic spectra, we identify all but a few of the previously unidentified significant absorption sp…

2009 Icarus
Cassini 13
Major Solar Energetic Particle Events of Solar Cycles 22 and 23: Intensities Close to the Streaming Limit
DOI: 10.1007/s11207-009-9463-1 Bibcode: 2009SoPh..260..407L

Lario, D.; Aran, A.; Decker, R. B.

It has been argued that the highest intensities measured near 1 AU during large solar energetic particle events occur in association with the passage of interplanetary shocks driven by coronal mass ejections, whereas the intensities measured early in the events (known as the prompt component) are bounded by a maximum intensity plateau known as the…

2009 Solar Physics
SOHO 13
New X-Ray Observations of the Old Nova CP Puppis and of the More Recent Nova V351 Puppis
DOI: 10.1088/0004-637X/690/2/1753 Bibcode: 2009ApJ...690.1753O

Mukai, K.; de Martino, D.; Orio, M. +2 more

We present X-ray observations of the field containing Nova Puppis 1942 (CP Pup) and Nova Puppis 1991 (V351 Pup), done with ASCA in 1998, and with XMM-Newton in 2005. The X-ray and UV luminosity of CP Pup seem to have remained approximately constant since the last X-ray observations of the 1980s, while the optical luminosity has decreased. The X-ra…

2009 The Astrophysical Journal
IUE XMM-Newton 13
Relative timing of substorm processes as derived from multifluid/multiscale simulations: Internally driven substorms
DOI: 10.1029/2008JA013750 Bibcode: 2009JGRA..114.9213W

Winglee, R. M.; Harnett, E.; Kidder, A.

The role of tail reconnection in initiating substorm onset remains highly controversial. Multifluid/multiscale simulations are used to examine this problem with the unique capability of being able to resolve ion skin depth and ion cyclotron processes within a very thin tail current sheet within a global magnetosphere. It is shown that, consistent …

2009 Journal of Geophysical Research (Space Physics)
Cluster 13
Emission and Absorption Properties of Low-Mass Type 2 Active Galaxies with XMM-Newton
DOI: 10.1088/0004-637X/705/2/1196 Bibcode: 2009ApJ...705.1196T

Ho, Luis C.; Thornton, Carol E.; Barth, Aaron J. +1 more

We present XMM-Newton observations of four low-redshift Seyfert galaxies selected to have low host luminosities (Mg > - 20 mag) and small stellar velocity dispersions (σ* <45 km s-1), which are among the smallest stellar velocity dispersions found in any active galaxies. These galaxies show weak or no broad o…

2009 The Astrophysical Journal
XMM-Newton 13
Multi-spacecraft Observations of CIR-Associated Ion Increases During the Ulysses 2007 Ecliptic Crossing
DOI: 10.1007/s11207-009-9356-3 Bibcode: 2009SoPh..256..409D

Dresing, Nina; Heber, Bernd; Gómez-Herrero, Raúl +3 more

The period between 21 June and 8 October, 2007 (Carrington rotations 2058 to 2061), comprising the Ulysses ecliptic plane crossing, was characterized by low solar activity. Excluding the small solar energetic particle events observed during July, the ion increases observed in the inner heliosphere between 100 keV/n and 10 MeV/n were associated wit…

2009 Solar Physics
Ulysses 13