Search Publications

The Purple Haze of η Carinae: Binary-induced Variability?
DOI: 10.1086/423341 Bibcode: 2004ApJ...610L.105S

Smith, Nathan; Gull, Theodore R.; Collins, Nicholas R. +1 more

Asymmetric variability in ultraviolet images of the Homunculus obtained with the Advanced Camera for Surveys/High Resolution Camera on the Hubble Space Telescope suggests that η Carinae is indeed a binary system. Images obtained before, during, and after the recent ``spectroscopic event'' in 2003.5 show alternating patterns of bright spots and sha…

2004 The Astrophysical Journal
eHST 67
XMM-Newton Observations of the Galactic Supernova Remnant CTB 109 (G109.1-1.0)
DOI: 10.1086/425353 Bibcode: 2004ApJ...617..322S

Sasaki, Manami; Smith, Randall K.; Plucinsky, Paul P. +3 more

We present the analysis of the X-ray Multimirror Mission (XMM-Newton) European Photon Imaging Camera (EPIC) data of the Galactic supernova remnant (SNR) CTB 109 (G109.1-1.0). CTB 109 is associated with the anomalous X-ray pulsar (AXP) 1E 2259+586 and has an unusual semicircular morphology in both the X-ray and the radio and an extended X-ray brigh…

2004 The Astrophysical Journal
XMM-Newton 67
Rapid Penumbral Decay following Three X-Class Solar Flares
DOI: 10.1086/382188 Bibcode: 2004ApJ...601L.195W

Liu, C.; Qiu, J.; Wang, H. +3 more

We show strong evidence that penumbral segments decayed rapidly and permanently right after three X-class solar flares. Two of the three events occurred very recently in NOAA Active Region 10486, an X17 flare on 2003 October 28 and an X10 flare on 2003 October 29. The third X2.3 flare was observed in solar active region NOAA AR 9026 on 2000 June 6…

2004 The Astrophysical Journal
SOHO 67
RHESSI Observations of a Simple Large X-Ray Flare on 2003 November 3
DOI: 10.1086/423371 Bibcode: 2004ApJ...611L..53L

Liu, Wei; Liu, Siming; Jiang, Yan Wei +1 more

We present data analysis and interpretation of a simple X-class flare observed with RHESSI on 2003 November 3. In contrast to other X-class flares observed previously, this flare shows a very simple morphology with well-defined looptop (LT) and footpoint (FP) sources. The almost monotonic upward motion of the LT source and increase in separation o…

2004 The Astrophysical Journal
SOHO 67
Solar Cycle 23: An Anomalous Cycle?
DOI: 10.1086/421104 Bibcode: 2004ApJ...609.1140D

de Toma, Giuliana; White, Oran R.; Chapman, Gary A. +3 more

The latest SOHO VIRGO total solar irradiance (TSI) time series is analyzed using new solar variability measures obtained from full-disk solar images made at the San Fernando Observatory and the Mg II 280 nm index. We discuss the importance of solar cycle 23 as a magnetically simpler cycle and a variant from recent cycles. Our results show the cont…

2004 The Astrophysical Journal
SOHO 67
The Mid-Infrared Luminosity Function of Galaxies in the European Large Area Infrared Space Observatory Survey Southern Fields
DOI: 10.1086/420963 Bibcode: 2004ApJ...609..122P

Pozzi, F.; Franceschini, A.; Serjeant, S. +7 more

We present the first determination of the 15 µm luminosity function of galaxies from the European Large Area ISO Survey (ELAIS) southern fields. We have adopted a new criterion to separate the quiescent, nonevolving and the starburst, evolving populations based on the ratio of mid-infrared to optical luminosity. Strong evolution is suggested…

2004 The Astrophysical Journal
ISO 67
The Variable Quiescence of Centaurus X-4
DOI: 10.1086/380194 Bibcode: 2004ApJ...601..474C

Campana, S.; Mereghetti, S.; Stella, L. +2 more

Centaurus X-4 is one of the best-studied low-mass neutron star transients in quiescence. Thanks to XMM-Newton's large throughput, Centaurus X-4 was observed at the highest signal-to-noise ratio ever. This allowed us to discern rapid (>100 s), large (45%+/-7% rms in the 10-4 to 1 Hz range) intensity variability, especially at low ener…

2004 The Astrophysical Journal
XMM-Newton 66
Time Dependence in Relativistic Collisionless Shocks: Theory of the Variable ``Wisps'' in the Crab Nebula
DOI: 10.1086/381568 Bibcode: 2004ApJ...603..669S

Spitkovsky, Anatoly; Arons, Jonathan

We describe results from time-dependent numerical modeling of the collisionless reverse shock terminating the pulsar wind in the Crab Nebula. We treat the upstream relativistic wind as composed of ions and electron-positron plasma embedded in a toroidal magnetic field, flowing radially outward from the pulsar in a sector around the rotational equa…

2004 The Astrophysical Journal
eHST 66
The Ultraviolet Extinction Curve of Intraclump Dust in Taurus (TMC-1): Constraints on the 2175 Å Bump Absorber
DOI: 10.1086/380837 Bibcode: 2004ApJ...602..291W

Gordon, Karl D.; Whittet, D. C. B.; Clayton, Geoffrey C. +1 more

Ultraviolet extinction curves for three early-type stars that sample dust in the Taurus dark cloud in the vicinity of TMC-1 are analyzed to examine the contribution of internal (intraclump) dust to the total line-of-sight extinction. One of our selected targets samples only dust in the ``diffuse-screen'' component of the cloud, where the dust grai…

2004 The Astrophysical Journal
IUE 66
Helioseismic Mapping of the Magnetic Canopy in the Solar Chromosphere
DOI: 10.1086/424996 Bibcode: 2004ApJ...613L.185F

Finsterle, W.; McIntosh, S. W.; Jefferies, S. M. +2 more

We determine the three-dimensional topography of the magnetic canopy in and around active regions by mapping the propagation behavior of high-frequency acoustic waves in the solar chromosphere.

2004 The Astrophysical Journal
SOHO 66