Search Publications

Inferring Photospheric Velocity Fields Using a Combination of Minimum Energy Fit, Local Correlation Tracking, and Doppler Velocity
DOI: 10.1086/528363 Bibcode: 2008ApJ...677..751R

Longcope, D. W.; Ravindra, B.; Abbett, W. P.

The minimum energy fit (MEF), a velocity inversion technique, infers all components of the photospheric velocity that are consistent with the induction equation. From the set of consistent velocity fields, it selects the smallest overall flow speed by minimizing a kinetic energy functional. If partial velocity information is available from other m…

2008 The Astrophysical Journal
SOHO 26
A Study of the ρ Ophiuchi Cloud: Mapping the Distribution and the Motions of Interstellar Gas
DOI: 10.1086/587132 Bibcode: 2008ApJ...679..512S

Welty, Daniel E.; Snow, Theodore P.; Destree, Joshua D.

Guest Investigator results from Hipparcos, combined with high-resolution optical spectra obtained with the Anglo-Australian Observatory, Kitt Peak National Observatory, and McDonald Observatory, are used to create a three-dimensional map of the stars and several interstellar gas components in the ρ Oph cloud complex. Many principal gas components …

2008 The Astrophysical Journal
Hipparcos eHST 26
A Comparison among Solar Diameter Measurements Carried Out from the Ground and outside Earth's Atmosphere
DOI: 10.1086/524680 Bibcode: 2008ApJ...676..651D

Thuillier, G.; Djafer, D.; Sofia, S.

The solar diameter has been measured since the 17th century, using different methods and instruments, and without a clear strategy of measurement, which could explain the lack of coherence between the results obtained. The present study confirms that the discrepancies between solar diameter measurements are mostly due to differences in instrumenta…

2008 The Astrophysical Journal
SOHO 26
UV and Radio Observations of the Coronal Shock Associated with the 2002 July 23 Coronal Mass Ejection Event
DOI: 10.1086/528839 Bibcode: 2008ApJ...677..683M

Mancuso, S.; Avetta, D.

We report on the analysis of a fast coronal mass ejection (CME)-driven shock observed on 2002 July 23 with the Ultraviolet Coronagraph Spectrometer (UVCS) on board the Solar and Heliospheric Observatory (SOHO). The CME was first detected in white light by the Large Angle and Spectrometric Coronagraph Experiment (LASCO), and shock-associated type I…

2008 The Astrophysical Journal
SOHO 26
Validating Time-Distance Far-Side Imaging of Solar Active Regions through Numerical Simulations
DOI: 10.1086/592721 Bibcode: 2008ApJ...689.1373H

Zhao, Junwei; Kosovichev, Alexander G.; Hartlep, Thomas +1 more

Far-side imaging using time-distance helioseismology methods is assessed using numerically generated artificial data. The data are generated using direct numerical simulations of acoustic oscillations in a spherical solar model. Localized variations of the sound speed in the surface and subsurface layers are used to model the perturbations associa…

2008 The Astrophysical Journal
SOHO 26
Isotopic Ratios in Titan's Atmosphere from Cassini CIRS Limb Sounding: HC3N in the North
DOI: 10.1086/590534 Bibcode: 2008ApJ...681L.109J

Irwin, P. G. J.; Teanby, N. A.; Flasar, F. M. +8 more

This Letter reports the first detection of the three 13C isotopologues of HC3N on Titan, from Cassini Composite Infrared Spectrometer (CIRS) infrared spectra. The data are limb spectra taken at latitudes N54°-N69° in 2006 and 2007 when HC3N was enhanced in the north. Using a new line list for the ν5 band…

2008 The Astrophysical Journal
Cassini 26
Low-Frequency Lyα Power Spectra Observed by UVCS in a Polar Coronal Hole
DOI: 10.1086/588093 Bibcode: 2008ApJ...677L.137B

Bemporad, A.; Poletto, G.; Matthaeus, W. H.

The occurrence of f-1 noise in interplanetary magnetic fields (in the 1 × 10-5 to 1 × 10-4 Hz band) and other plasma parameters has now been known for about 20 years and has been recently identified also in the photospheric magnetic fields. However, the relationship between interplanetary and solar fluctuation spec…

2008 The Astrophysical Journal
SOHO 26
A Kiloparsec-Scale X-Ray Jet in the BL Lac Source S5 2007+777
DOI: 10.1086/589918 Bibcode: 2008ApJ...684..862S

Maraschi, L.; Cheung, C. C.; Tavecchio, F. +2 more

X-ray jets in AGNs are commonly observed in FR II and FR I radio galaxies, but rarely in BL Lac objects, most probably due to their orientation close to the line of sight and the ensuing foreshortening effects. Only three BL Lac objects are known so far to contain a kpc-scale X-ray jet. In this paper we present the evidence for the existence of a …

2008 The Astrophysical Journal
eHST 25
Exploratory Study of the X-Ray Properties of Quasars with Intrinsic Narrow Absorption Lines
DOI: 10.1086/529426 Bibcode: 2008ApJ...677..863M

Charlton, Jane C.; Eracleous, Michael; Misawa, Toru +1 more

We have used archival Chandra and XMM-Newton observations of quasars hosting intrinsic narrow UV absorption lines (intrinsic NALs) to carry out an exploratory survey of their X-ray properties. Our sample consists of three intrinsic NAL quasars and one "mini-BAL" quasar, plus four quasars without intrinsic absorption lines for comparison. These wer…

2008 The Astrophysical Journal
XMM-Newton 25
Lensing Probabilities for Spectroscopically Selected Galaxy-Galaxy Strong Lenses
DOI: 10.1086/589958 Bibcode: 2008ApJ...685...57D

Keeton, Charles R.; Dobler, Gregory; Bolton, Adam S. +1 more

Spectroscopic galaxy-galaxy lens searches are presently the most prolific method of identifying strong lens systems in large data sets. We study the probabilities associated with these lens searches, namely the probability of identifying a candidate with rogue [O II] emission lines in a galaxy's spectrum, and the probability that the candidate wil…

2008 The Astrophysical Journal
eHST 25