Search Publications

A Multi-Wavelength Investigation of the Unidentified Gamma-Ray Source HESS J1708-410
DOI: 10.1088/0004-637X/707/2/1717 Bibcode: 2009ApJ...707.1717V

Funk, Stefan; Hinton, Jim; Van Etten, Adam

We report on recent XMM-Newton observations, archival radio continuum and CO data, and spectral energy distribution (SED) modeling of the unidentified Galactic plane source HESS J1708-410. No significant extended X-ray emission is observed, and we place an upper limit of 3.2 × 10-13 erg cm-2 s-1 in the 2-4 keV rang…

2009 The Astrophysical Journal
XMM-Newton 6
Evidence of the radio-quiet hard X-ray precursor of the 13 December 2006 solar flare
DOI: 10.1016/j.asr.2008.09.009 Bibcode: 2009AdSpR..43..680Z

Zimovets, I. V.; Struminsky, A. B.; Gros, M.

We report multi-wavelength investigation of the pre-impulsive phase of the 13 December 2006 X-class solar flare. We use hard X-ray data from the anticoincidence system of spectrometer onboard INTEGRAL (ACS) jointly with soft X-ray data from the GOES-12 and Hinode satellites. Radio data are from Nobeyama and Learmonth solar observatories and from t…

2009 Advances in Space Research
Hinode 6
Magnetic helicity and active filament configuration
DOI: 10.1051/0004-6361/200912425 Bibcode: 2009A&A...506..895R

Poedts, S.; Romano, P.; Zuccarello, F. P. +2 more

Context: The role of magnetic helicity in active filament formation and destabilization is still under debate.
Aims: Although active filaments usually show a sigmoid shape and a twisted configuration before and during their eruption, it is unclear which mechanism leads to these topologies. In order to provide an observational contribution to c…

2009 Astronomy and Astrophysics
SOHO 6
Water ice crystallinity and grain sizes on Dione
DOI: 10.1016/j.icarus.2009.04.034 Bibcode: 2009Icar..203..553N

Brown, R. H.; Buratti, B. J.; Jaumann, R. +3 more

Saturn's satellite Dione is becoming an increasingly important object in the outer Solar System, as evidence for its current activity accumulates. Infrared observations of the surface can provide clues to the history of the body and currently active processes. Using data from the Cassini Visual and Infrared Mapping Spectrometer (VIMS), we perform …

2009 Icarus
Cassini 6
Multiwavelength study of M33's giant HII regions NGC 588 and NGC 592
DOI: 10.1111/j.1365-2966.2009.14490.x Bibcode: 2009MNRAS.394.1847U

Drissen, Laurent; Úbeda, Leonardo

We present a detailed multiwavelength photometric study of giant HII regions NGC 592 and NGC 588 in the nearby small spiral galaxy M33. We use data taken with the Wide Field and Planetary Camera 2 (WFPC2) on board the Hubble Space Telescope (HST). We detect several massive stars in both ionizing clusters. Six Wolf-Rayet (WR) stars are known to exi…

2009 Monthly Notices of the Royal Astronomical Society
eHST 6
High-Resolution Near-Infrared Images of the T Tauri Binary System XZ Tauri
DOI: 10.1093/pasj/61.6.1271 Bibcode: 2009PASJ...61.1271H

Pyo, Tae-Soo; Tamura, Motohide; Hayashi, Masahiko +8 more

We present a high-resolution (∼0.1'' = 14AU) H-band image of XZ Tau, a 0.3''-separated classical T Tauri binary system, taken with the Coronagraphic Imager with Adaptive Optics (CIAO) on the Subaru Telescope. We found a scattered light nebula extending to ∼2.4'' from the secondary, XZ Tau S, in the northeast region of the binary. Its surface brigh…

2009 Publications of the Astronomical Society of Japan
eHST 6
Modelling of mirror mode structures as propagating slow magnetosonic solitons
DOI: 10.5194/angeo-27-4379-2009 Bibcode: 2009AnGeo..27.4379S

Stasiewicz, K.; Cheng, C. Z.

Cluster measurements in the magnetosheath with spacecraft separations of 2000 km indicate that magnetic pulsations interpreted as mirror mode structures are not frozen in plasma flow, but do propagate with speeds of up to ~50 km/s. Properties of these pulsations are shown to be consistent with propagating slow magnetosonic solitons. By using nonli…

2009 Annales Geophysicae
Cluster 6
Cusp observations during a sequence of fast IMF BZ reversals
DOI: 10.5194/angeo-27-2721-2009 Bibcode: 2009AnGeo..27.2721C

Pitout, F.; Davies, J. A.; Lockwood, M. +6 more

In recent years, a large number of papers have reported the response of the cusp to solar wind variations under conditions of northward or southward Interplanetary Magnetic Field (IMF) Z-component (BZ). These studies have shown the importance of both temporal and spatial factors in determining the extent and morphology of the cusp and t…

2009 Annales Geophysicae
Cluster 6
Clustering of Red Galaxies Around the z = 1.53 Quasar 3C 270.1
DOI: 10.1088/0004-637X/695/1/724 Bibcode: 2009ApJ...695..724H

Wilkes, Belinda J.; Fazio, G. G.; Ashby, M. L. N. +6 more

In the paradigm of hierarchical galaxy formation, luminous radio galaxies mark mass assembly peaks that should contain clusters of galaxies. Observations of the z = 1.53 quasar 3C 270.1 with the Spitzer Space Telescope at 3.6-24 µm and with the 6.5 m MMT in the z' and Y bands allow the detection of potential cluster members via photometric r…

2009 The Astrophysical Journal
eHST 6
Suzaku Observations of SN 1987A
DOI: 10.1093/pasj/61.4.895 Bibcode: 2009PASJ...61..895S

Haberl, Frank; Hasinger, Günther; Sturm, Richard +2 more

We report on Suzaku observations of SN1987A in the Large Magellanic Cloud, performed in 2005 November and 2006 June. The observations provide medium resolution X-ray spectra during the phase of the interaction between the supernova blast wave and the inner circumstellar ring. The Suzaku observations complement XMM-Newton and Chandra observations a…

2009 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 6