Zobrazeno 1 - 10
of 45
pro vyhledávání: '"Stüwe, J. A."'
Autor:
Tozzi, G. P., Patriarchi, P., Boehnhardt, H., Vincent, J. -B., Licandro, J., Kolokolova, L., Schulz, R., Stüwe, J.
Comet 67P/Churyumov-Gerasimenko is the main target of ESA's Rosetta mission and will be encountered in May 2014. As the spacecraft shall be in orbit the comet nucleus before and after release of the lander {\it Philae}, it is necessary necessary to k
Externí odkaz:
http://arxiv.org/abs/1105.0329
Autor:
Manfroid, J., Jehin, E., Hutsemékers, D., Cochran, A., Zucconi, J. -M., Arpigny, C., Schulz, R., Stüwe, J. A., Ilyin, I.
Our aim is to determine the isotopic ratios {$^{12}$C/$^{13}$C}{} and {$^{14}$N/$^{15}$N}{} in a variety of comets and link these measurements to the formation and evolution of the solar system. The {$^{12}$C/$^{13}$C}{} and {$^{14}$N/$^{15}$N}{} iso
Externí odkaz:
http://arxiv.org/abs/0907.0311
Autor:
Oosterbroek, T., Cognard, I., Golden, A., Verhoeve, P., Martin, D. D. E., Erd, C., Schulz, R., Stuewe, J. A., Stankov, A., Ho, T.
The Crab pulsar emits across a large part of the electromagnetic spectrum. Determining the time delay between the emission at different wavelengths will allow to better constrain the site and mechanism of the emission. We have simultaneously observed
Externí odkaz:
http://arxiv.org/abs/0806.3634
Autor:
Meech, K. J., Ageorges, N., Arpigny, C., Ates, A., Aycock, J., Bagnulo, S., Bailey, J., Barber, R., Barrera, L., Barrena, R., Bauer, J. M., Belton, M. J. S., Bensch, F., Bhattacharya, B., Biver, N., Blake, G., Bockelée-Morvan, D., Boehnhardt, H., Bonev, B. P., Bonev, T., Buie, M. W., Burton, M. G., Butner, H. M., Cabanac, R., Campbell, R., Campins, H., Capria, M. T., Carroll, T., Chaffee, F., Charnley, S. B., Cleis, R., Coates, A., Cochran, A., Colom, P., Conrad, A., Coulson, I. M., Crovisier, J., deBuizer, J., Dekany, R., de Léon, J., Russo, N. Dello, Delsanti, A., DiSanti, M., Drummond, J., Dundon, L., Etzel, P. B., Farnham, T. L., Feldman, P., Fernández, Y. R., Filipovic, M. D., Fisher, S., Fitzsimmons, A., Fong, D., Fugate, R., Fujiwara, H., Fujiyoshi, T., Furusho, R., Fuse, T., Gibb, E., Groussin, O., Gulkis, S., Gurwell, M., Hadamcik, E., Hainaut, O., Harker, D., Harrington, D., Harwit, M., Hasegawa, S., Hergenrother, C. W., Hirst, P., Hodapp, K., Honda, M., Howell, E. S., Hutsemékers, D., Iono, D., Jackson, W., Jehin, E., Jiang, Z. J., Jones, G. H., Jones, P. A., Kadono, T., Kamath, U. W., Käufl, H. U., Kasuga, T., Kawakita, H., Kelley, M. S., Kerber, F., Kidger, M., Kinoshita, D., Knight, M., Lara, L., Larson, S. M., Lederer, S., Levasseur-Regourd, A. C., Li, J. Y., Licandro, J., Lisse, C. M., LoCurto, G., Lovell, A. J., Lowry, S. C., Lyke, J., Lynch, D., Ma, J., Magee-Sauer, K., Maheswar, G., Manfroid, J., Marco, O., Martin, P., Melnick, G., Miller, S., Miyata, T., Moriarty-Schieven, G. H., Moskovitz, N., Mueller, B. E. A., Mumma, M. J., Muneer, S., Neufeld, D. A., Ootsubo, T., Osip, D., Pandea, S. K., Pantin, E., Paterno-Mahler, R., Patten, B., Penprase, B. E., Peck, A., Petitas, G., Pinilla-Alonso, N., Pittichova, J., Pompei, E., Prabhu, T. P., Qi, C., Rao, R., Rauer, H., Reitsema, H., Rodgers, S. D., Rodriguez, P., Ruane, R., Ruch, G., Rujopakarn, W., Sahu, D. K., Sako, S., Sakon, I., Samarasinha, N., Sarkissian, J. M., Saviane, I., Schirmer, M., Schultz, P., Schulz, R., Seitzer, P., Sekiguchi, T., Selman, F., Serra-Ricart, M., Sharp, R., Snell, R. L., Snodgrass, C., Stallard, T., Stecklein, G., Sterken, C., Stüwe, J. A., Sugita, S., Sumner, M., Suntzeff, N., Swaters, R., Takakuwa, S., Takato, N., Thomas-Osip, J., Thompson, E., Tokunaga, A. T., Tozzi, G. P., Tran, H., Troy, M., Trujillo, C., Van Cleve, J., Vasundhara, R., Vazquez, R., Vilas, F., Villanueva, G., von Braun, K., Vora, P., Wainscoat, R. J., Walsh, K., Watanabe, J., Weaver, H. A., Weaver, W., Weiler, M., Weissman, P. R., Welsh, W. F., Wilner, D., Wolk, S., Womack, M., Wooden, D., Woodney, L. M., Woodward, C., Yamashita, T., Yang, B., Yokogawa, S., Zook, A. C., Zauderer, A., Zhao, X., Zhou, X.
Publikováno v:
Science, 2005 Oct . 310(5746), 265-269.
Externí odkaz:
https://www.jstor.org/stable/3842647
Autor:
Arpigny, Claude, Jehin, Emmanuël, Manfroid, Jean, Hutsemékers, Damien, Schulz, Rita, Stüwe, J. A., Zucconi, Jean-Marc, Ilyin, Ilya
Publikováno v:
Science, 2003 Sep 01. 301(5639), 1522-1524.
Externí odkaz:
https://www.jstor.org/stable/3835076
Publikováno v:
Astronomy and Astrophysics, 398, 345-352
Scopus-Elsevier
Scopus-Elsevier
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::5f9e566ad37fbd9016d97f6b08394b0e
https://hdl.handle.net/1887/7531
https://hdl.handle.net/1887/7531
Autor:
Manfroid E. Jehin D. Hutsemékers A. Cochran J.-M. Zucconi C. Arpigny R. Schulz And J.A. Stüwe., J.
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 432, pp.L5-L8
Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 432, pp.L5-L8
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::dc06bbea69d4551b7bfeedf4dca8b23a
https://hal.archives-ouvertes.fr/hal-00019619
https://hal.archives-ouvertes.fr/hal-00019619
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
NASA Astrophysics Data System
We report broad-band X-ray measurements of the Be star Gamma Cassiopeiae by the BeppoSAX X-ray astronomy satellite. The observations took place on 1998 July, 18-23. The 0.1-200 keV X-ray spectrum is reasonably well fit by an optically thin thermal pl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79583976a71906048fc2fecc57542f6b
http://arxiv.org/abs/astro-ph/9905245
http://arxiv.org/abs/astro-ph/9905245