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Plasma Waves Near Reconnection Sites
Bibcode: 2006LNP...687..251V

André, M.; Vaivads, A.; Treumann, R. A. +1 more

2006 Geospace Electromagnetic Waves and Radiation
Cluster 15
High-Ionization Forbidden Lines in the UV Spectrum of AG Draconis
DOI: 10.1086/506584 Bibcode: 2006ApJ...650.1091Y

Young, P. R.; Dupree, A. K.; Espey, B. R. +1 more

High-ionization forbidden lines from Ca VII, Fe VII, Mg V, Mg VI, Mg VII, and Si VII are found in recent Hubble Space Telescope STIS ultraviolet spectra of the symbiotic star AG Draconis. These species have ionization potentials between 99 and 205 eV, which are unexpected due to the high density (~1010 cm-3) of the AG Dra neb…

2006 The Astrophysical Journal
eHST 15
Large Silicon Abundance in Photodissociation Regions
DOI: 10.1086/499801 Bibcode: 2006ApJ...640..383O

Nakagawa, Takao; Onaka, Takashi; Tomono, Daigo +3 more

We have made one-dimensional raster scan observations of the ρ Oph and σ Sco star-forming regions with two spectrometers (SWS and LWS) on board the ISO. In the ρ Oph region, [Si II] 35 µm, [O I] 63 µm, 146 µm, [C II] 158 µm, and the H2 pure rotational transition lines S(0) to S(3) are detected, and the photodisso…

2006 The Astrophysical Journal
ISO 15
Radio and X-ray observations of an exceptional radio flare in the extreme z = 4.72 blazar GBB1428+4217
DOI: 10.1111/j.1365-2966.2006.10173.x Bibcode: 2006MNRAS.368..844W

Fabian, A. C.; Worsley, M. A.; Pooley, G. G. +1 more

We report on the extreme behaviour of the high-redshift blazar GBB1428+4217 at z = 4.72. A continued programme of radio measurements has revealed an exceptional flare in the light curve, with the 15.2-GHz flux density rising by a factor of ~3 from ~140 to ~430 mJy in a rest-frame time-scale of only ~4 months - much larger than any previous flares …

2006 Monthly Notices of the Royal Astronomical Society
XMM-Newton 15
Astrochemistry: Complex organic matter in Titan's aerosols?
DOI: 10.1038/nature05417 Bibcode: 2006Natur.444E...6B

Biemann, K.

2006 Nature
Huygens 15
Spectral shape of the UV ionizing background and O VI absorbers at z ∼ 1.5 towards HS 0747+4259
DOI: 10.1051/0004-6361:20053834 Bibcode: 2006A&A...449....9R

Reimers, D.; Hagen, H. -J.; Lopez, S. +5 more

Aims.We report on high resolution spectra of the bright QSO HS 0747+4259 (z_em = 1.90, V = 15.8) observed to search for intermediate redshift O VI absorption systems.Methods.The spectra were obtained by means of the Space Telescope Imaging Spectrograph (STIS) at the Hubble Space Telescope (HST) and the High Resolution Echelle Sp…

2006 Astronomy and Astrophysics
eHST 15
The Recent Star Formation in NGC 6822 from Hubble Space Telescope Imaging
DOI: 10.1086/504919 Bibcode: 2006AJ....132..378B

Bianchi, Luciana; Efremova, Boryana V.

We present Hubble Space Telescope WFPC2 and STIS imaging of the low-metallicity galaxy NGC 6822, performed as part of a study of the young stellar populations in the galaxies of the Local Group. Eleven WFPC2 pointings, with some overlap, cover two regions extending over 19 and 13 arcmin2, respectively, off the galaxy center. The filters…

2006 The Astronomical Journal
eHST 15
Non-self-similar scaling of plasma sheet and solar wind probability distribution functions of magnetic field fluctuations
DOI: 10.1029/2006JA011820 Bibcode: 2006JGRA..11111209W

Balogh, A.; Khurana, K. K.; Kistler, L. M. +5 more

Solar wind magnetometer and plasma data and magnetometer data acquired by Cluster in the magnetospheric plasma sheet are employed to construct probability distribution functions (PDFs) of magnetic field fluctuations over various temporal and spatial scales. This technique, often used in analysis of laboratory plasmas, is used to look for intermitt…

2006 Journal of Geophysical Research (Space Physics)
Cluster 15
Adaptive-Optics-Assisted Near-Infrared Spectroscopy of SVS 13 and Its Jet
DOI: 10.1086/499557 Bibcode: 2006ApJ...639..969D

Smith, M. D.; Ray, T. P.; Nisini, B. +5 more

We present long-slit H- and K-band spectroscopy of the low-mass outflow source SVS 13, obtained with the adaptive-optics-assisted imager-spectrometer NACO on the VLT. With a spatial resolution of <0.25" and a pixel scale of 0.027", we precisely establish the relative offsets of H2, [Fe II], CO, H I, and Na I components from the sourc…

2006 The Astrophysical Journal
eHST 15
The Brave New World of Binary Star Studies
DOI: 10.1007/s10509-006-9069-0 Bibcode: 2006Ap&SS.304....5G

Guinan, Edward F.; Engle, Scott G.

In this paper we discuss some of the new and exciting developments in the study of binary stars. Recent technological advances (such as CCDs) now make it possible (even easy) to study faint, astrophysically important binaries that in the past could only be done with large 4 + meter class telescopes. Also, the panoramic nature of CCDs (and the use …

2006 Astrophysics and Space Science
eHST 15