Swift is a first-of-its-kind multiwavelength transient observatory for GRB astronomy. It has the optimum capabilities for the next breakthroughs in determining...
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PublicationThe Swift Gamma-Ray Burst Mission
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PublicationThe System Parameters of the Polars MR SER and ST LMi
We obtain the Na I lambda 8183,8195 absorption line radial velocity curves for the polars ST LMi and MR Ser, from which we find the semi-amplitudes to be Kabs...
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PublicationThe Tc Trend In The Zetta Reticuli System: N Spectra – N Trends.
It is suggested that the chemical abundance trend with the condensation temperature, Tc , can be a signature of rocky planet formation or accretion. Recently, a...
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PublicationThe Temperature of Massive Stars
Not Available
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PublicationThe temporal behaviour of seeing
Using a large amount of data gathered during previous seeing campaign at ORM, we analyse the temporal evolution of seeing in order to find out whether...
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PublicationThe Temporal Evolution of Linear Fast and Alfvén MHD Waves in Solar Coronal Arcades
The excitation and temporal evolution of fast and Alfvén magnetohydrodynamic oscillations in a two-dimensional coronal arcade are investigated. The approach is...
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PublicationThe Tenerife CMB Fluctuation Experiment: Progress to Date
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PublicationThe thirty gigahertz instrument receiver for the Q-U-I Joint Tenerife experiment: Concept and experimental results
This paper presents the analysis, design, and characterization of the thirty gigahertz instrument receiver developed for the Q-U-I Joint Tenerife experiment...
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PublicationThe tip of the iceberg: the frequency content of the δ Sct star HD 50844 from CoRoT space photometry
It has been suggested that the detection of a wealth of very low amplitude modes in δ Sct stars was only a matter of signal-to-noise ratio. Access to this...