Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Cody Gerhartz"'
Autor:
A. F. J. Moffat, Jim Fuller, Gregg A. Wade, Werner W. Weiss, Coralie Neiner, Jason F. Rowe, Adam Popowicz, Rainer Kuschnig, Ludwik Lembryk, Gerald Handler, Herbert Pablo, Noel D. Richardson, Wayne L. Oswald, B. Buysschaert, A. D. Bratcher, Jennifer J. Greco, Andrzej Pigulski, Kevin K. Hardegree-Ullman, Cody Gerhartz, Tahina Ramiaramanantsoa
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2017, 467 (2), pp.2494-2503. ⟨10.1093/mnras/stx207⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 467 (2), pp.2494-2503. ⟨10.1093/mnras/stx207⟩
Monthly Notices of the Royal Astronomical Society, 2017, 467 (2), pp.2494-2503. ⟨10.1093/mnras/stx207⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 467 (2), pp.2494-2503. ⟨10.1093/mnras/stx207⟩
{\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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::71367b0baa7a4532f9f06620aca126e8
https://hal.science/hal-02189628/document
https://hal.science/hal-02189628/document
Autor:
Luqian Wang, Jon E. Bjorkman, A. D. Bratcher, Alex C. Carciofi, Robert Klement, Kevin K. Hardegree-Ullman, Karen S. Bjorkman, Cody Gerhartz, Nicholas A. Dulaney, Noel D. Richardson, Jesica Trucks, Jennifer J. Greco, Wayne L. Oswald, Nancy D. Morrison, Ludwik Lembryk
The late-type Be star $\beta$ CMi is remarkably stable compared to other Be stars that have been studied. This has led to a realistic model of the outflowing Be disk by Klement et al. These results showed that the disk is likely truncated at a finite
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::63e6742e533e9fbfb06192e58093bc4d
http://arxiv.org/abs/1701.05201
http://arxiv.org/abs/1701.05201
Autor:
G. C. Anupama, Jussi Harmanen, Simone Zaggia, Cody Gerhartz, Raffaella Margutti, R. Mancini, S. Benetti, Nancy Elias-Rosa, A. Morales-Garoffolo, Morgan Fraser, Ron Arbour, Ryan Chornock, Stephen J. Smartt, Kuntal Misra, Marco Berton, Étienne Artigau, D. K. Sahu, L. Tomasella, Karen S. Bjorkman, K. Itagaki, Rubina Kotak, G. Cortini, Noel D. Richardson, Massimo Turatto, J. Polshaw, S. Taubenberger, F. Martinelli, A. Dimai, P. Ochner, Daniel J. Patnaude, A. Pastorello, Michel Dennefeld, F. Briganti, Dan Milisavljevic, Giacomo Terreran, Enrico Cappellaro, T. Boles, F. Ciabattari, Leonardo Tartaglia, Peter J. Brown
Publikováno v:
BASE-Bielefeld Academic Search Engine
This is the final version of the article. It first appeared from Oxford University Press via http://dx.doi.org/10.1093/mnras/stw2253
Supernova (SN) 2015bh (or SNhunt275) was discovered in NGC 2770 on 2015 February with an absolute magnitude of M
Supernova (SN) 2015bh (or SNhunt275) was discovered in NGC 2770 on 2015 February with an absolute magnitude of M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cfb87523ccac5ed477823173a14205c8