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A new γ-ray pulsar: PSR 0740-28

Lu, Tan; Ma, Yu-qian; Song, Li-ming

We made a period folding analysis on two sets of COS-B observations and obtained a clearly pulsed phase structure in the γ-ray photons from the direction of PSR 0740-28. The phase diagrams from the two different data sets have a similar structure and the period and period rate are close to radio expectations. The probability of the two phase struc…

Is There a Drift of Anomalous Cosmic Ray Particles? Measurements of the ULYSSES EPAC Instrument

Fränz, M.; Keppler, E.; Quenby, J. J. +5 more

The Ulysses Data System.

Tranquille, C.

Following the successful launch of the Ulysses spacecraft in October 1990, there is great expectation that the scientific data return from the first out-of-ecliptic mission will be considerable. The aim of the Ulysses Data System (UDS) is to facilitate the exchange of data between the instrument teams, thereby encouraging scientific research into …

Comparison of Recurrent Ion Events Using Uiysses HI-SCALE and EPAC and Voyager LECP Data

Krupp, N.; Krimigis, S. M.; Keppler, E. +3 more

Ulysses' Race to the Pole: Symposium Summary

Lee, Martin A.

This paper reproduces the Symposium Summary presentation at the 28th ESLAB Symposium on The High Latitude Heliosphere. The summary is not comprehensive but with considerable latitude covers the highlights of the conference. Featured are the observations of the high-speed wind from the growing southern polar coronal hole, new measurements of the in…

Ultraviolet Standard luminosity profiles for normal galaxies

Longo, G.; Capaccioli, M.; Rifatto, A.

Satelliten vertiefen Verständnis über das interstellare Gas.

de Boer, K. S.

Space research of interstellar gas: COPERNICUS, IUE, IRAS, ROSAT.

ESA/IUE under the Web

Barylak, M.; Ponz, J. D.; de la Fuente, A. +1 more

The Periodic Variation of 1 and >92 MeV Proton Fluxes at High Latitudes

Anglin, J. D.

IUE Echelle observations of the photospheres and circumstellar environments of hot white dwarfs

Holberg, J. B.

For well over a decade, narrow, interstellar-like features have been observed in the high resolution ME spectra of many hot white dwarfs. It is now clear that these features originate in at least two different environments. In many of the hottest white dwarfs these features are formed in the stellar photosphere by trace amounts of key ions of C, N…