Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Oswald, W. L."'
Autor:
Pablo, Herbert, Richardson, N. D., Fuller, J., Rowe, J., Moffat, A. F. J., Kuschnig, R., Popowicz, A., Handler, G., Neiner, C., Pigulski, A., Wade, G. A., Weiss, W., Buysschaert, B., Ramiaramanantsoa, T., Bratcher, A. D., Gerhartz, C. J., Greco, J. J., Hardegree-Ullman, K., Lembryk, L., Oswald, W. L.
{\iota} Ori is a well studied massive binary consisting of an O9 III + B1 III/IV star. Due to its high eccentricity (e = 0.764) and short orbital period (P orb = 29.13376 d), it has been considered to be a good candidate to show evidence of tidal eff
Externí odkaz:
http://arxiv.org/abs/1703.02086
Autor:
Pablo, Herbert, Richardson, N. D., Fuller, J., Rowe, J., Moffat, A. F. J., Kuschnig, R., Popowicz, A., Handler, G., Neiner, C., Pigulski, A., Wade, G. A., Weiss, W., Buysschaert, B., Ramiaramanantsoa, T., Bratcher, A. D., Gerhartz, C. J., Greco, J. J., Hardegree-Ullman, K., Lembryk, L., Oswald, W. L.
�� Ori is a well studied massive binary consisting of an O9 III + B1 III/IV star. Due to its high eccentricity (e = 0.764) and short orbital period (P orb = 29.13376 d), it has been considered to be a good candidate to show evidence of tidal effe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3e4bf6a83a9996b4c7597775d35f6354
Autor:
Oswald, W. L.
Publikováno v:
Proceedings of the Association of Official Seed Analysts of North America, 1919 Jan 01. 11, 38-41.
Externí odkaz:
https://www.jstor.org/stable/23430584
Autor:
Oswald, W. L.
Publikováno v:
Proceedings of the Association of Official Seed Analysts of North America, 1923 Jul 01. 14/15, 141-145.
Externí odkaz:
https://www.jstor.org/stable/23431353
Autor:
Pablo, Herbert, Richardson, N. D., Fuller, J., Rowe, J., Moffat, A. F. J., Kuschnig, R., Popowicz, A., Handler, G., Neiner, C., Pigulski, A., Wade, G. A., Weiss, W., Buysschaert, B., Ramiaramanantsoa, T., Bratcher, A. D., Gerhartz, C. J., Greco, J. J., Hardegree-Ullman, K., Lembryk, L., Oswald, W. L.
Publikováno v:
Monthly Notices of the Royal Astronomical Society; May2017, Vol. 467 Issue 2, p2494-2503, 10p