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The EXOSAT and Einstein observations of 1E0630 + 178 ('Geminga') as complementary data sets
Caraveo, P. A.; Bignami, G. F.; Mereghetti, S. +1 more
Data for the soft X-ray source 1E0630 + 178 are now available from four independent measurements of the Einstein and EXOSAT missions. These are presented and compared in the light of the different characteristics and energy response of the different X-ray imaging detectors used (IPC, LE 1, LE 2). The time variability on medium (hours) time scale i…
CA II K emission in Canopus.
Bappu, M. K. V.; Mekkaden, M. V.; Rao, N. K.
The changes in the Ca II K line profile of the F0 supergiant Canopus have been studied from the high dispersion coude spectrograms obtained since 1975. The emission in the core of the line is variable in a timescale of few days. Similar activity seems to be occurring in Mg II h and k lines also. This is attributed to the variability in the appeara…
Three gamma-ray sources with large angular sizes
Li, T. -P.
From an analysis of the data from the gamma-ray satellite COS-B and from radio measurements of CO molecules, it appears probable that the three gamma-ray sources 2CG 036+01, 218-00, 235-01 are either isolated giant molecular clouds or superpositions of clouds unresolved by the detector.
An ultraviolet identification list for the AP star IOTA Cassiopeiae.
Jasinski, M.; Woszczyk, A.
The authors present a detailed identification of the absorption lines in the ultraviolet spectrum of ι Cas. The list contains 412 lines. The identified lines belong mainly to iron and chromium. Also many lines of manganese are present.
Background-sensitive event selection in the search for gamma-ray sources
Özel, M. E.; Mayer-Haßelwander, H. A.
Poor angular resolution of present day gamma ray telescopes (1° at 100 MEV) together with the complicated gamma ray sky structures at compareable angular extents and poor statistics available necessitate the selection of those gammas which will increase the observable signal from a suspected source. A method for such a selection using the pre-know…
Exosat observations of the supernova remnant W49B.
Jones, L. R.
The transition layer of eleven late-type stars.
Montesinos, B.; Rego, M.; Fernandez-Figueroa, M. J.
Far UV-spectra of eleven F, G, and K stars of different luminosity class have been studied. Si IV, C IV, and N V emission line fluxes have been used to obtain parameters for the transition region. The stars of the sample have been classified according to the activity level. Using two abundance criteria the gaseous pressure upper limits have been c…
Evidence for an increasing 59 S period in the X-ray emission from Geminga
Caraveo, P. A.; Bignami, G. F.; Salotti, L.
Einstein Observatory and EXOSAT X-ray data from 1E0630 + 178 reveal an approximately 50-percent periodic emission at about 59 s or more. This confirms the early SAS-II and COS-B findings on 2CG 195 + 04 at E greater than 50 MeV and provides the temporal signature for the identification of Geminga. The observations, spanning over a decade (1973-198…
The EXOSAT mission - Status and early results
Taylor, B. G.; Peacock, A.; Andresen, R. D.
The status of the EXOSAT programme, during the calibration and performance verification phase, is summarised and some highlight results from this phase are presented.
X-ray astronomy: Milestone for EXOSAT
Watson, Mike