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The dispersion in the Cepheid period-luminosity relation and the consequences for the extragalactic distance scale
DOI: 10.1111/j.1365-2966.2004.07286.x Bibcode: 2004MNRAS.347.1011A

Shanks, Tom; Allen, Paul D.

Using published Hubble Space Telescope (HST) Cepheid data from 25 galaxies, we have found a correlation between the dispersion in the Cepheid period-luminosity (P-L) relation and host galaxy metallicity, which is significant at the ~3σ level in the V band. In the I band the correlation is less significant, although the tighter intrinsic dispersion…

2004 Monthly Notices of the Royal Astronomical Society
eHST 11
Cassini/VIMS observation of an Io post-eclipse brightening event
DOI: 10.1016/j.icarus.2004.05.012 Bibcode: 2004Icar..172..141B

Brown, R. H.; Baines, K. H.; Buratti, B. J. +10 more

During the Cassini-Jupiter flyby, VIMS observed Io at different phase angles, both in full sunlight and in eclipse. By using the sunlight measurements, we were able to produce phase curves in the visual through all the near infrared wavelengths covered by the VIMS instrument (0.85-5.1 µm). The phase angle spanned from ∼2° to ∼120°. The measu…

2004 Icarus
Cassini 11
FUSE Observations of Highly Ionized Gas in the Vela Supernova Remnant
DOI: 10.1086/383135 Bibcode: 2004ApJ...606..900S

Blair, William P.; Nichols, Joy S.; Slavin, Jonathan D.

We present Far Ultraviolet Spectroscopic Explorer (FUSE) data on O VI absorption lines observed toward nine stars behind the Vela supernova remnant (SNR). The O VI observations are compared with International Ultraviolet Explorer (IUE) observations of C IV absorption toward the same stars. All of these stars are B stars, which generally have compl…

2004 The Astrophysical Journal
IUE 11
Global control of merging by the interplanetary magnetic field: Cluster observations of dawnside flank magnetopause reconnection
DOI: 10.1029/2003JA010346 Bibcode: 2004JGRA..10912203E

Balogh, A.; RèMe, H.; André, M. +7 more

Detailed Cluster observations of flank magnetopause reconnection are presented for two events on the Northern and the Southern Hemispheric dawnside flanks when the interplanetary magnetic field (IMF) clock angle ? = arctan(By/Bz) is within ∼45° of the equatorial plane. The event selection is based on the relative proximity be…

2004 Journal of Geophysical Research (Space Physics)
Cluster 11
Evidence for the Same Hot Plasma after Coronal Mass Ejection Events, in Both Remote and In Situ Observations
DOI: 10.1086/425136 Bibcode: 2004ApJ...613L.173P

Poletto, G.; Ko, Y. -K.; Bemporad, Alessandro +4 more

We present here evidence for highly ionized Fe observed both in the corona, in the aftermath of a coronal mass ejection, and, after propagation, in situ. The apparent source temperature is greater than 6 MK. To our knowledge, this is the first time that such an unambiguous identification has been made. This detection complements studies correlatin…

2004 The Astrophysical Journal
SOHO Ulysses 11
A serendipitous survey for galaxy clusters by the XMM-Newton Survey Science Center
DOI: 10.1016/j.asr.2003.04.073 Bibcode: 2004AdSpR..34.2604S

Elvis, M.; Watson, M. G.; Lamer, G. +6 more

We describe the initial results of a programme to detect and identify extended X-ray sources found serendipitously in XMM-Newton observations. We have analyzed 186 EPIC-PN images at high galactic latitude with a limiting flux of 1 × 10 -14 erg cm -2 s -1 and found 62 cluster candidates. Thanks to the enhanced sensi…

2004 Advances in Space Research
XMM-Newton 11
Mid-infrared imaging and modelling of the dust shell around post-AGB star HD 187885 (IRAS 19500-1709)
DOI: 10.1111/j.1365-2966.2004.08483.x Bibcode: 2004MNRAS.355L..17C

Gledhill, T. M.; Clube, K. L.

We present 10- and 20-µm images of IRAS 19500-1709 taken with the mid-infrared camera, OSCIR, mounted on the Gemini North Telescope. An extended circumstellar envelope is detected, with the N-band image indicating an elongation in a north-east-south-west direction. We use a dust radiation transport code to fit the spectral energy distributio…

2004 Monthly Notices of the Royal Astronomical Society
IUE 11
A New Way to Model the Solar Oscillation ℓ−ν Power Spectrum
DOI: 10.1023/B:SOLA.0000031404.13076.73 Bibcode: 2004SoPh..220..347J

Jefferies, Stuart M.; Vorontsov, Sergei V.

We present a new approach for the precise and accurate forward modeling of the solar oscillation ℓ−ν power spectrum. The approach is designed to provide the basis for a streamlined solar seismic inversion without measurements of the p-mode frequencies. The new strategy represents a paradigm change in how information is extracted from the oscillati…

2004 Solar Physics
SOHO 11
The Nature of Close Companions of the BL Lacertae Objects 1ES 0502+675 and 1ES 1440+122
DOI: 10.1086/423169 Bibcode: 2004ApJ...613..747G

Falomo, R.; Treves, A.; Urry, C. M. +2 more

We report on deep radio images and optical spectroscopy of two BL Lac objects that have very close compact companions. The two targets, 1ES 0502+675 and 1ES 1440+122, were selected from the Hubble Space Telescope imaging survey of 110 BL Lacs as candidates for possible gravitational lensing. The new observations clearly demonstrate that the compan…

2004 The Astrophysical Journal
eHST 11
The composite starburst/AGN nature of the superwind galaxy NGC 4666
DOI: 10.1051/0004-6361:20041128 Bibcode: 2004A&A...427...35P

Palazzi, E.; Cappi, M.; Franceschini, A. +6 more

We report the discovery of a Compton-thick AGN and of intense star-formation activity in the nucleus and disk, respectively, of the nearly edge-on superwind galaxy NGC 4666. Spatially unresolved emission is detected by BeppoSAX only at energies <10 keV, whereas spatially resolved emission from the whole disk is detected by XMM-Newton. A promine…

2004 Astronomy and Astrophysics
XMM-Newton 10