Titlebook: Astrotomography; Indirect Imaging Met Henri M.J. Boffin,Jan Cuypers,Danny Steeghs Book 2001 Springer-Verlag Berlin Heidelberg 2001 Accretio

死亡率

The Geometrical Configuration of Polars and Possible Reconstruction Artefacts of Eclipse Mapping Me streams is more complicated than that of accretion disks in non-magnetic systems, it is essential to gain knowledge about the geometrical con.guration of such a system. Here, I give a summary of the parameters with which the geometry can be described. I present some reconstruction artefacs that can be the results of wrong geometrical parameters.

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Spot Mapping in Cool Stars,eview I outline the signal enhancement and indirect imaging techniques available for mapping spots on stellar surfaces. I review recent developments in the use of starspots as tracers of surface differential rotation, and discuss the way in which starspot lifetimes appear to scale with stellar luminosity class.

消毒

Astrotomography978-3-540-45339-0Series ISSN 0075-8450 Series E-ISSN 1616-6361

核心

liposuction

lobster

https://doi.org/10.1007/978-3-0348-4121-4systems. Many examples show that the lines are composed not only from (symmetrical) disc emission, but that additional contribution is provided by isolated, i.e. asymmetric emission sources, distorting the original line profile. In this paper, we study the distribution of these additional components with several system parameters.

流行

periodontitis

Compiling and Running Java Programs,eview I outline the signal enhancement and indirect imaging techniques available for mapping spots on stellar surfaces. I review recent developments in the use of starspots as tracers of surface differential rotation, and discuss the way in which starspot lifetimes appear to scale with stellar luminosity class.

Acumen

Doppler Tomography,on over the binary. I begin with a discussion of the basic principles behind Doppler tomography, including a comparison of the relative merits of maximum entropy regularisation versus filtered back-projection for implementing the inversion. Following this I discuss the issue of noise in Doppler imag

Lineage

Mapping the Peculiar Binary GP Com,observed in previous UV and optical data. We find that the central spike contributes to the flare spectra indicating that its origin is probably the compact object. We also detect that the central spike moves with orbital phase following an S-wave pattern. The radial velocity semiamplitude of the S-