Zobrazeno 1 - 10
of 543
pro vyhledávání: '"Funk B."'
Publikováno v:
2015MNRAS.453.2308S
This paper is devoted to study the circumstances favourable to detect Trojan planets in close binary-star-systems by the help of eclipse timing variations (ETVs). To determine the probability of the detection of such variations with ground based tele
Externí odkaz:
http://arxiv.org/abs/1608.00784
Publikováno v:
2016MNRAS.460.3598S
This paper is devoted to study the circumstances favourable to detect circumstellar and circumbinary planets in well detached binary-star-systems using eclipse timing variations (ETVs). We investigated the dynamics of well detached binary star system
Externí odkaz:
http://arxiv.org/abs/1608.00764
Autor:
Kislyakova, K. G., Pilat-Lohinger, E., Funk, B., Lammer, H., Fossati, L., Eggl, S., Schwarz, R., Boudjada, M. Y., Erkaev, N. V.
We suggest an additional possible plasma source to explain part of the phenomena observed for the transiting hot Jupiters WASP-12b and HD 189733b in their ultraviolet (UV) light curves. In the proposed scenario, material outgasses from the molten sur
Externí odkaz:
http://arxiv.org/abs/1605.02507
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 414, Issue 3, pp. 2763-2770 (2011)
In close eclipsing binaries, measurements of the variations in binary's eclipse timing may be used to infer information about the existence of circumbinary objects. To determine the possibility of the detection of such variations with CoRoT and Keple
Externí odkaz:
http://arxiv.org/abs/1101.1994
Publikováno v:
Astron.Astrophys.410:L13-L16,2003
Using numerical methods we thoroughly investigate the dynamical stability in the region between the two planets found in HD 74156. The two planets with minimum masses 1.56 M_JUP (HD 74156b) and 7.5 M_JUP (HD 74156c), semimajor axes 0.276 AU and 3.47
Externí odkaz:
http://arxiv.org/abs/astro-ph/0307009
Publikováno v:
Astron.Astrophys. 398 (2003) L1-L4
The recently discovered planetary system in the binary GamCep was studied concerning its dynamical evolution. We confirm that the orbital parameters found by the observers are in a stable configuration. The primary aim of this study was to find stabl
Externí odkaz:
http://arxiv.org/abs/astro-ph/0211289
Autor:
HEGRA collaboration, Padilla, L., Funk, B., Krawczynski, H., Contreras, J. L., Moralejo, A., Aharonian, F., Akhperjanian, A. G., Barrio, J. A., Beteta, J. G., Cortina, J., Deckers, T., Fonseca, V., Gebauer, H. -J., Gonzalez, J. C., Heinzelmann, G., Horns, D., Kornmayer, H., Lindner, A., Lorenz, E., Magnussen, N., Meyer, H., Mirzoyan, R., Petry, D., Plaga, R., Prahl, J., Prosch, C., Rauterberg, G., Rhode, W., Roehring, A., Sahakian, V., Samorski, M., Schmele, D., Stamm, W., Wiebel-Sooth, B., Willmer, M., Wittek, W.
A search for gamma-ray bursts (GRBs) above 20 TeV within the field of view (1 sr) of the HEGRA AIROBICC Cherenkov array (29N, 18W, 2200 m a.s.l.) has been performed using data taken between March 1992 and March 1993. The search is based on an all-sky
Externí odkaz:
http://arxiv.org/abs/astro-ph/9807342
Publikováno v:
Astropart.Phys. 9 (1998) 97-103
The energy spectrum of Mkn501 in the TeV energy regime, as measured by the HEGRA (High Energy Gamma Ray Astronomy) Cerenkov telescopes during its low state in 1995/96 and during a fraction of the 1997 outburst in the TeV energy regime, is shown to pl
Externí odkaz:
http://arxiv.org/abs/astro-ph/9802308
Autor:
Krawczynski, H., Funk, B., collaboration, the HEGRA, Barthelmy, S., Butterworth, P., Cline, T., Gehrels, N., Kouveliotou, C., Fishman, J., Meegan, C.
The HEGRA experiment is an air shower detector system for the study of neutral and charged cosmic rays in the energy range between 500 GeV to 10 PeV. Here we give an overview of how the HEGRA detector is used to search for TeV gamma-radiation associa
Externí odkaz:
http://arxiv.org/abs/astro-ph/9611044
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