Search Publications

Latitudinal extent of large-scale structures in the solar wind
DOI: 10.5194/angeo-21-1331-2003 Bibcode: 2003AnGeo..21.1331E

McComas, D. J.; Riley, P.; Elliott, H. A.

Comparison of solar wind observations from the ACE spacecraft, in the ecliptic plane at ~ 1 AU, and the Ulysses spacecraft as it orbits over the Sun's poles, provides valuable information about the latitudinal extent and variation of solar wind structures in the heliosphere. While qualitative comparisons can be made using average properties observ…

2003 Annales Geophysicae
Ulysses 3
XESS: An XMM Extended Source Survey
DOI: 10.1002/asna.200310037 Bibcode: 2003AN....324..138S

Saxton, R. D.; Neumann, D. M.; Denby, M. +1 more

2003 Astronomische Nachrichten
XMM-Newton 3
The XMM-Newton SSC serendipitous cluster survey
DOI: 10.1002/asna.200310055 Bibcode: 2003AN....324..156L

Elvis, M.; Watson, M. G.; Schwope, A. +2 more

2003 Astronomische Nachrichten
XMM-Newton 2
Interstellar Silicon Abundance
Bibcode: 2003AcA....53..379G

Gnacinski, P.

We present 34 measurements of silicon gas phase column densities in the interstellar medium. We have used spectra containing the SiII 1808 Ang line which were obtained with the Goddard High Resolution Spectrograph (GHRS) aboard the Hubble Space Telescope (HST). Extinction curve parameters are determined for analyzed lines of sight and relation bet…

2003 Acta Astronomica
IUE eHST 2
First IBIS results on the high energy emission of Cygnus X-2
DOI: 10.1051/0004-6361:20031421 Bibcode: 2003A&A...411L.395N

Santangelo, A.; Capitanio, F.; Ubertini, P. +4 more

The bright low-mass X-ray binary Cyg X-2 was in the field of view of the IBIS telescope during the early Cygnus region observations, executed during the INTEGRAL Performance Verification Phase. The data presented are spanning about one week and cover the rising edge of one of the two peaks of the ~82 day cycle of the Cyg X-2 light curve. The IBIS …

2003 Astronomy and Astrophysics
INTEGRAL 2
Multipolar Bubbles, Point-Symmetry, and Jets in Dying Stars
Bibcode: 2003RMxAC..15...17S

Sahai, R.; Morris, M. R.

The imaging of young planetary and pre-planetary nebulae (YPNe and PPNe) with unprecedented high angular resolution and dynamic range using the Hubble Space Telescope (HST), has shown that most of these objects are highly aspherical, with complex multipolar morphologies. The complexity, organization and symmetry of the morphological structures has…

2003 Revista Mexicana de Astronomia y Astrofisica Conference Series
eHST 2
The mean stellar parameters from IUE and hipparcos data
DOI: 10.1016/S0273-1177(02)00633-6 Bibcode: 2003AdSpR..31..399N

Niemczura, E.; Cugier, H.; Daszyńska, J.

2003 Advances in Space Research
Hipparcos IUE 2
6C radio galaxies at z∼1: the influence of radio power on the alignment effect
DOI: 10.1016/S1387-6473(03)00035-6 Bibcode: 2003NewAR..47..255I

Best, Philip N.; Inskip, Katherine J.; Longair, Malcolm S.

Powerful radio galaxies often display enhanced optical/UV continuum emission and extended emission line regions, elongated and aligned with the radio jet axis. The expansion of the radio source strongly affects the gas clouds in the surrounding IGM, and the kinematic and ionization properties of the extended emission line regions display considera…

2003 New Astronomy Reviews
eHST 2
Erratum: The ISO-SWS spectrum of planetary nebula NGC 7027
DOI: 10.1051/0004-6361:20030797 Bibcode: 2003A&A...406..175B

Pottasch, S. R.; Beintema, D. A.; Bernard-Salas, J. +1 more

Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands and UK) and with the participation of ISAS and NASA.

2003 Astronomy and Astrophysics
ISO 2
Fine structure of the polar cusp as deduced from the plasma wave and plasma measurements
DOI: 10.1016/S0273-1177(03)90269-9 Bibcode: 2003AdSpR..32..315B

Sauvaud, J. -A.; Santolik, O.; Parrot, M. +7 more

Plasma waves are one of the most significant features of plasma. They are a very sensitive indicator of the boundaries and inner structure of different regions in space plasmas. The data gathered onboard Interball 1 and Magion 4 in the polar cusp indicate that plasma wave intensity changes very rapidly with a characteristic period of the order of …

2003 Advances in Space Research
Cluster 2