Zobrazeno 1 - 10
of 45
pro vyhledávání: '"Mochnacki, S."'
Autor:
Pablo, H., Whittaker, G. N., Popowicz, A., Mochnacki, S. M., Kuschnig, R., Grant, C. C., Moffat, A. F. J., Rucinski, S. M., Matthews, J. M., Schwarzenberg-Czerny, A., Handler, G., Weiss, W. W., Baade, D., Wade, G. A., Zoclonska, E., Ramiaramanantsoa, T., Unterberger, M., Zwintz, K., Pigulski, A., Rowe, J., Koudelka, O., Orleanski, P., Pamyatnykh, A., Neiner, C., Wawrzaszek, R., Marciniszyn, G., Romano, P., Wozniak, G., Zawistowski, T., Zee, R. E.
BRITE (BRIght Target Explorer) Constellation, the first nanosatellite mission applied to astrophysical research, is a collaboration among Austria, Canada and Poland. The fleet of satellites (6 launched, 5 functioning) performs precise optical photome
Externí odkaz:
http://arxiv.org/abs/1608.00282
The blue straggler phenomenon is not yet well explained by current theory; however, evolutionary models of star clusters call for a good knowledge of it. Here we try to understand the possible formation scenario of HD 73666, a blue straggler member o
Externí odkaz:
http://arxiv.org/abs/0911.1874
Autor:
Vinko, J., Takats, K., Sarneczky, K., Szabo, Gy. M., Meszaros, Sz., Csorvasi, R., Szalai, T., Gaspar, A., Pal, A., Csizmadia, Sz., Kospal, A., Racz, M., Kun, M., Csak, B., Furesz, G., DeBond, H., Grunhut, J., Thomson, J., Mochnacki, S., Koktay, T.
Publikováno v:
Mon.Not.Roy.Astron.Soc.369:1780-1796,2006
New BVRI photometry and optical spectroscopy of the Type IIp supernova 2004dj in NGC 2403, obtained during the first year since discovery, are presented. The progenitor cluster, Sandage 96, is also detected on pre-explosion frames. The light curve in
Externí odkaz:
http://arxiv.org/abs/astro-ph/0604230
Autor:
Vinko, J., Blake, R. M., Sarneczky, K., Csak, B., Furesz, G., Csizmadia, Sz., Kiss, L. L., Szabo, Gy. M., Szabo, R., DeBond, H., de Robertis, M. M., Thomson, J. R., Mochnacki, S. W.
Publikováno v:
Astron.Astrophys.427:453-464,2004
New optical photometric and spectroscopic data of the bright hypernova SN 2002ap are presented. The obtained BVRI light curves as well as the optical spectra agree well with other published data series. The distance has been inferred by applying the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408571
Autor:
Rucinski, S. M., Capobianco, C. C., Lu, W., DeBond, H., Thomson, J. R., Mochnacki, S. W., Blake, R. M., Ogloza, W., Stachowski, G., Rogoziecki, P.
Radial-velocity measurements and sine-curve fits to the orbital velocity variations are presented for the seventh set of ten close binary systems: V410 Aur, V523 Cas, QW Gem, V921 Her, V2357 Oph, V1130 Tau, HN UMa, HX UMa, HD 93917, NSV 223. All syst
Externí odkaz:
http://arxiv.org/abs/astro-ph/0302399
Autor:
Rucinski, S. M., Lu, W., Capobianco, C., Mochnacki, S. W., Blake, R. M., Thomson, J. R., Ogloza, W., Stachowski, G.
Radial-velocity measurements and sine-curve fits to the orbital velocity variations are presented for the sixth set of ten close binary systems: SV Cam, EE Cet, KR Com, V410 Cyg, GM Dra, V972 Her, ET Leo, FS Leo, V2388 Oph, II UMa. All systems except
Externí odkaz:
http://arxiv.org/abs/astro-ph/0201213
Radial-velocity measurements and sine-curve fits to the orbital velocity variations are presented for the fifth set of ten close binary systems: V376 And, EL Aqr, EF Boo, DN Cam, FN Cam, V776 Cas, SX Crv, V351 Peg, EQ Tau, KZ Vir. All systems are dou
Externí odkaz:
http://arxiv.org/abs/astro-ph/0106160
We present medium resolution (lambda/Delta lambda = 2500) optical spectroscopy of SN 1999by in NGC 2841 made around its light maximum. The depth ratio of the two Si II features at 5800 AA and 6150 AA being R(SiII) approx. 0.63 at maximum indicates th
Externí odkaz:
http://arxiv.org/abs/astro-ph/0103034
Autor:
Mochnacki, S. W.
A method for the computer synthesis of theoretical light curves and like profiles for close binary stars in general has been developed and applied to the W Ursae Majoris stars. The geometry has been calculated using the centrally-condensed Roche mode
Externí odkaz:
http://hdl.handle.net/10092/8167
Autor:
Kuschnig, R., Pigulski, A., Moffat, A. F. J., Matthews, J. M., Zwintz, K., Baade, D., Handler, G., Weiss, W. W., Wade, G. A., Rucinski, S. M., Pablo, H., Koudelka, O., Smolec, R., Popowicz, A., Neiner, Coralie, Daszynska-Daszkiewicz, J., Lovekin, C., St-Louis, N., Pamyatnykh, A. A., Rowe, J., Orleanski, P., Mochnacki, S., Schwarzenberg-Czerny, A.
Publikováno v:
The Astronomer's telegram
The Astronomer's telegram, 2018
The Astronomer's telegram, 2018
International audience; One of the five satellites in BRITE-Constellation (http://www.brite-constellation.at/) was obtaining time-series optical photometry of the star HD 92063, only 2 arcmin from the 'Possible, Very Bright Galactic Nova ASASSN-18fv'
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::a16b3e917edb3269275a875332c543c1
https://hal.archives-ouvertes.fr/hal-02323694
https://hal.archives-ouvertes.fr/hal-02323694