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The population of massive stars in R136 from HST/FOC UV observations
Leitherer, Claus; Nota, Antonella; de Marchi, Guido +2 more
New ultraviolet (λ≃1300 A, λ≃3400 A),HST FOC observations have been used to derive the UV color-magnitude diagram (CMD) of R136, with the main scientific goal of studying the upper end of the stellar mass function at ultraviolet wavelengths where the color degeneracy encountered in visual CMDs is less severe. The CMD has been compared to a set of …
The Decay Phase of the March-April, 1991 Low-Energy Particle Events Observed at Ulysses and Earth
Simnett, G. M.; Lanzerotti, L. J.; Armstrong, T. P. +2 more
Multiwavelength astronomy using ESIS
Giommi, P.; Ansari, S. G.
We present results on multi-frequency astronomy obtained using the European Space Information System, ESIS. ESIS is an ESA service designed to access, manipulate and combine archival data from a number of remote archives in the fields of Astronomy and Space Physics. The examples presented here include plots of radio-to-X-ray energy distribution of…
Multiwavelength monitoring of active galactic nuclei
Urry, C. M.
Recent multiwavelength monitoring of active galactic nuclei (AGN), particularly with the IUE satellite, has produced extraordinary advances in our understanding of the energy-generation mechanism(s) in the central engine and of the structure of the surrounding material. Examples discussed here include both ordinary AGN and blazars (the collective …
Ion Abundances in Solar Event at 5.3 AU
Tappin, S. J.; Lanzerotti, L. J.; Gold, R. E. +2 more
Ulysses Observations of Solar Wind Proton and Alpha Particle Temperatures and Anisotropies from 1 to 5 AU
McComas, D. J.; Goldstein, B. E.; Bame, S. J. +3 more
Analysis of COS-B and HEAO-B satellite data of the pulsar Geminga
Wu, Mei; Ma, Lin; Ma, Yu-qian +4 more
We have made timing and spectral analyses of COS-B and HEAO-B satellite data of the pulsar Geminga and our results further confirm that Geminga is a pulsar with a strong γ emission and a weak X emission.
Multiwavelength Searches for the Counterpart to the May 1 1992 Gamma-Ray Burst
Cline, T.; Hurley, K.; Kouveliotou, C. +9 more
UV and X-ray emission in the interacting binary U Cephei.
Gonzalez-Riestra, R.; Guinan, E. F.; Gimenez, A.
The active close binary U Cep has been monitored in the ultraviolet, using IUE, during 1.25 orbital cycles. The emission spectrum at the bottom of the primary total eclipse confirms earlier suggestions of an unexpected absence of the Hell 1640 A line. Stronger than expected emission in some other lines like NV, CII, CIV or AlIII, indicative of hot…
Search for short bursts of gamma-ray emission in spark chamber data: application to COS-B
Buccheri, R.; Maccarone, M. C.; Fry, W. F.
We describe an analysis method aimed to the detection of short (<1000 s) bursts in the emission of gamma-ray sources using spark chamber data. The method utilizes a maximum likelihood technique which looks for accumulations of photons, compatible with the point spread function of the experiment, within the whole observing time and the field-of-…