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The Orbit and Albedo of Trans-Neptunian Binary (58534) 1997 CQ29
DOI: 10.1086/424535 Bibcode: 2004AJ....128.2547N

Noll, Keith S.; Stephens, Denise C.; Grundy, Will M. +2 more

We have measured the separations and position angles of the two components of the binary trans-Neptunian object (58534) 1997 CQ29 at eight epochs. From these data we are able to constrain the orbit and mass of this binary system. The best-fitting orbit has an orbital period of P=312+/-3 days. The orbital eccentricity is e=0.45+/-0.03 an…

2004 The Astronomical Journal
eHST 30
Oscillations in the Umbral Atmosphere
DOI: 10.1023/B:SOLA.0000035065.10112.fc Bibcode: 2004SoPh..221..237B

Foley, C. R.; Fredvik, T.; Kjeldseth-Moe, O. +2 more

The results of simultaneous observations of oscillations in the chromosphere, transition region, and corona above nine sunspots are presented. The data are obtained through coordinated observing with the Solar and Heliospheric Observatory — SOHO and the Transition Region And Coronal Explorer — TRACE. Oscillations are detected above each umbra. The…

2004 Solar Physics
SOHO 30
XMM-Newton EPIC and Optical Monitor observations of Her X-1 over the 35-d beat period
DOI: 10.1111/j.1365-2966.2004.07660.x Bibcode: 2004MNRAS.350..506Z

Hailey, Charles J.; Ramsay, Gavin; Zane, Silvia +2 more

We present the results of a series of XMM-Newton European Photon Imaging Camera (EPIC) and Optical Monitor observations of Her X-1, spread over a wide range of the 35-d precession period. We confirm that the spin modulation of the neutron star is weak or absent in the low state - in marked contrast to the main or short-on states. During the states…

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton 30
Recent advances in the long-wavelength radio physics of the Sun
DOI: 10.1016/j.pss.2004.09.016 Bibcode: 2004P&SS...52.1399G

Gopalswamy, N.

Solar radio bursts at long wavelengths provide information on solar disturbances such as coronal mass ejections (CMEs) and shocks at the moment of their departure from the Sun. The radio bursts also provide information on the physical properties (density, temperature and magnetic field) of the medium that supports the propagation of the disturbanc…

2004 Planetary and Space Science
SOHO 30
Iron line spectroscopy of NGC 4593 with XMM-Newton: where is the black hole accretion disc?
DOI: 10.1111/j.1365-2966.2004.07909.x Bibcode: 2004MNRAS.352..205R

Kaiser, Mary Elizabeth; Brenneman, Laura W.; Wilms, Jörn +1 more

We present an analysis of the 2-10 keV XMM-Newton/EPIC-pn spectrum of the Seyfert-1 galaxy NGC 4593. Apart from the presence of two narrow emission lines corresponding to the Kα lines of cold and hydrogen-like iron, this spectrum possesses a power-law form to within ~3-5 per cent. There is a marked lack of spectral features from the relativistic r…

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton 30
Flow shear near the boundary of the plasma sheet observed by Cluster and Geotail
DOI: 10.1029/2003JA010174 Bibcode: 2004JGRA..109.5204N

Balogh, A.; RèMe, H.; Fazakerley, A. N. +13 more

We report on the transient strong flow shear (large northward/southward electric field) events accompanied by energetic ion beams and localized field-aligned currents observed at the boundary of the premidnight plasma sheet by Cluster in the Northern Hemisphere and Geotail in the Southern Hemisphere. The events took place associated with plasma sh…

2004 Journal of Geophysical Research (Space Physics)
Cluster 30
XMM-Newton confirmation of a warm absorber in the z= 4.4 blazar PMN J0525-3343
DOI: 10.1111/j.1365-2966.2004.07634.x Bibcode: 2004MNRAS.350..207W

Iwasawa, K.; Fabian, A. C.; Celotti, A. +2 more

We present the analysis and results from a series of XMM-Newton observations of the distant blazar PMN J0525-3343 at a redshift of 4.4. The X-ray spectrum shows a spectral flattening below ~1 keV, confirming earlier results from ASCA and BeppoSAX. The spectrum is well fitted by a power-law continuum with either a spectral break or absorption; no s…

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton 30
A young binary brown dwarf in the R-CrA star formation region
DOI: 10.1051/0004-6361:20035954 Bibcode: 2004A&A...424..213B

Demarco, R.; Martín, E. L.; Bouy, H. +5 more

We present imaging and spectroscopic observations with HST (WFPC2, ACS/HRC and STIS), VLT (FORS2) and Keck (HIRES) of the dM 8 ultra-cool dwarf DENIS-P J185950.9-370632, located in the R-CrA region. The presence of lithium absorption at 670.8 nm and the strong Hα emission indicate a young age and a sub-stellar mass. Our diffract…

2004 Astronomy and Astrophysics
ISO eHST 30
Period-luminosity relations for Galactic Cepheid variables with independent distance measurements
DOI: 10.1111/j.1365-2966.2004.07595.x Bibcode: 2004MNRAS.349.1130N

Ngeow, Chow-Choong; Kanbur, Shashi M.

In this paper, we derive the period-luminosity (PL) relation for Galactic Cepheids with recent independent distance measurements from open cluster, Barnes-Evans surface brightness, interferometry and Hubble Space Telescope astrometry techniques. Our PL relation confirms the results from recent works, which showed that the Galactic Cepheids follow …

2004 Monthly Notices of the Royal Astronomical Society
eHST 30
XMM-Newton spectral and timing analysis of the faint millisecond pulsars PSR J0751+1807 and PSR J1012+5307
DOI: 10.1051/0004-6361:20040069 Bibcode: 2004A&A...419..269W

Kramer, M.; Webb, N. A.; Barret, D. +3 more

We present XMM-Newton MOS imaging and PN timing data of the faint millisecond pulsars PSR J0751+1807 and PSR J1012+5307. We find 46 sources in the MOS field of view of PSR J0751+1807 searching down to an unabsorbed flux limit of 3 × 10-15 ergs cm-2 s-1 (0.2-1…

2004 Astronomy and Astrophysics
XMM-Newton 30