Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Mochnacki, S. W."'
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:
MOCHNACKI, S. W., WALKER, G. A. H.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1978 Aug 01. 90(536), 379-385.
Externí odkaz:
https://www.jstor.org/stable/40677216
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1984 Aug 01. 96(582), 663-666.
Externí odkaz:
https://www.jstor.org/stable/40678384
Autor:
MOCHNACKI, S. W., STARKMAN, G.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1985 Feb 01. 97(588), 151-152.
Externí odkaz:
https://www.jstor.org/stable/40678465
Publikováno v:
Publications of the Astronomical Society of the Pacific; August 1984, Vol. 96 Issue: 582 p663-663, 1p