Search Publications

The Hubble Space Telescope View of LINER Nuclei: Evidence for a Dual Population?
DOI: 10.1086/429612 Bibcode: 2005ApJ...625..716C

Chiaberge, Marco; Capetti, Alessandro; Macchetto, F. Duccio

We study a complete, distance-limited sample of 25 LINERs, 21 of which have been imaged with the Hubble Space Telescope. In nine objects we detect an unresolved nucleus. To study their physical properties, we compare the radio and optical properties of the nuclei of LINERs with those of other samples of local active galactic nuclei (AGNs), namely,…

2005 The Astrophysical Journal
eHST 65
First current density measurements in the ring current region using simultaneous multi-spacecraft CLUSTER-FGM data
DOI: 10.5194/angeo-23-1849-2005 Bibcode: 2005AnGeo..23.1849V

Balogh, A.; Dandouras, I.; Lucek, E. +7 more

The inner magnetosphere's current mapping is one of the key elements for current loop closure inside the entire magnetosphere. A method for directly computing the current is the multi-spacecraft curlometer technique, which is based on the application of Maxwell-Ampère's law. This requires the use of four-point magnetic field high resolution measur…

2005 Annales Geophysicae
Cluster 65
The first detection of [OIII] emission from high-redshift damped Lyman-α galaxies
DOI: 10.1111/j.1365-2966.2005.08838.x Bibcode: 2005MNRAS.358..985W

Fall, S. M.; Møller, P.; Weatherley, S. J. +3 more

We present the detection of [OIII] emission lines from the galaxies responsible for two high-redshift z > 1.75 damped Lyman-α (DLA) absorption lines. We find two sources of [OIII] emission corresponding to the z= 1.92 DLA absorber towards the quasar Q2206-1958, and we also detect [OIII] emission from the galaxy responsible for the z= 3.10 DLA a…

2005 Monthly Notices of the Royal Astronomical Society
eHST 65
Repeated X-Ray Flaring Activity in Sagittarius A*
DOI: 10.1086/497624 Bibcode: 2005ApJ...635.1095B

Grosso, N.; Porquet, D.; Ferrando, P. +5 more

Investigating the spectral and temporal characteristics of the X-rays coming from Sagittarius A* (Sgr A*) is essential to our development of a more complete understanding of the emission mechanisms in this supermassive black hole located at the center of our Galaxy. Several X-ray flares with varying durations and spectral features have already bee…

2005 The Astrophysical Journal
XMM-Newton 65
Oxygen-rich AGB stars with optically thin dust envelopes
DOI: 10.1051/0004-6361:20042296 Bibcode: 2005A&A...439..171H

Heras, A. M.; Hony, S.

The dust composition and dynamics of the circumstellar envelopes of oxygen-rich AGB stars with low mass-loss rates (5 × 10-8-10-5 M yr-1) have been investigated. We have analyzed the ISO-SWS spectra of twenty-eight oxygen-rich AGB stars with optically thin shells, and modelled the observations with the …

2005 Astronomy and Astrophysics
ISO 65
The Loopy Ultraviolet Line Profiles of RU Lupi: Accretion, Outflows, and Fluorescence
DOI: 10.1086/430075 Bibcode: 2005AJ....129.2777H

Herczeg, Gregory J.; Valenti, Jeff A.; Brown, Alexander +6 more

We present far-ultraviolet (FUV) spectra of the classical T Tauri star RU Lup covering the 912-1710 Å spectral range, as observed by the Hubble Space Telescope STIS and the Far Ultraviolet Spectroscopic Explorer satellite. We use these spectra, which are rich in emission and absorption lines, to probe both the accreting and outflowing gas. Absorpt…

2005 The Astronomical Journal
eHST 65
Pushing the ground-based limit: 14-µmag photometric precision with the definitive Whole Earth Telescope asteroseismic data set for the rapidly oscillating Ap star HR1217
DOI: 10.1111/j.1365-2966.2005.08807.x Bibcode: 2005MNRAS.358..651K

Kepler, S. O.; Kawaler, S. D.; Winget, D. E. +43 more

HR1217 is one of the best-studied rapidly oscillating Ap (roAp) stars, with a frequency spectrum of alternating even- and odd-l modes that are distorted by the presence of a strong, global magnetic field. Several recent theoretical studies have found that within the observable atmospheres of roAp stars the pulsation modes are magneto-acoustic with…

2005 Monthly Notices of the Royal Astronomical Society
Hipparcos 65
Modeling Complete Distributions with Incomplete Observations: The Velocity Ellipsoid from Hipparcos Data
DOI: 10.1086/431572 Bibcode: 2005ApJ...629..268H

Hogg, David W.; Johnston, Kathryn V.; Blanton, Michael R. +1 more

An algorithm is developed to model the three-dimensional velocity distribution function of a sample of stars using only measurements of each star's two-dimensional tangential velocity. The algorithm works with ``missing data'': it reconstructs the three-dimensional distribution from data (velocity measurements) that all have one dimension that is …

2005 The Astrophysical Journal
Hipparcos 65
Discovery of a 105 ms X-Ray Pulsar in Kesteven 79: On the Nature of Compact Central Objects in Supernova Remnants
DOI: 10.1086/430300 Bibcode: 2005ApJ...627..390G

Gotthelf, E. V.; Halpern, J. P.; Seward, F. D.

We report the discovery of 105 ms X-ray pulsations from the compact central object (CCO) in the supernova remnant Kes 79 using data acquired with the Newton X-Ray Multi-Mirror Mission (XMM-Newton). Two observations of the pulsar taken 6 days apart yield an upper limit on its spin-down rate of P˙<7×10-14 s s-1 and no eviden…

2005 The Astrophysical Journal
XMM-Newton 65
Non-parametric mass reconstruction of A1689 from strong lensing data with the Strong Lensing Analysis Package
DOI: 10.1111/j.1365-2966.2005.09372.x Bibcode: 2005MNRAS.362.1247D

Diego, J. M.; Broadhurst, T.; Benítez, N. +3 more

We present the mass distribution in the central area of the cluster A1689 by fitting over 100 multiply lensed images with the non-parametric Strong Lensing Analysis Package. The surface mass distribution is obtained in a robust way, finding a total mass of 0.25 × 1015h-1 Msolar within a 70-arcsec circle radius from…

2005 Monthly Notices of the Royal Astronomical Society
eHST 64