Zobrazeno 1 - 10
of 46
pro vyhledávání: '"Peng, Qiuhe"'
Some serious faults in error analysis of observations for SNIa have been found. Redoing the same error analysis of SNIa, by our idea, it is found that the average total observational error of SNIa is obviously greater than $0.55^m$, so we can't decid
Externí odkaz:
http://arxiv.org/abs/1201.3866
Autor:
Appourchaux, Thierry, Burston, Raymond, Chen, Yanbei, Cruise, Michael, Dittus, Hansjoerg, Foulon, Bernard, Gill, Patrick, Gizon, Laurent, Klein, Hugh, Klioner, Sergei, Kopeikin, Sergei, Krueger, Hans, Laemmerzahl, Claus, Lobo, Alberto, Luo, Xinlian, Margolis, Helen, Ni, Wei-Tou, Paton, Antonio Pulido, Peng, Qiuhe, Peters, Achim, Rasel, Ernst, Ruediger, Albrecht, Samain, Etienne, Selig, Hanns, Shaul, Diana, Sumner, Timothy, Theil, Stephan, Touboul, Pierre, Turyshev, Slava, Wang, Haitao, Wang, Li, Wen, Linqing, Wicht, Andreas, Wu, Ji, Zhang, Xiaomin, Zhao, Cheng
Publikováno v:
Exper.Astron.23:491-527,2009
ASTROD I is a planned interplanetary space mission with multiple goals. The primary aims are: to test General Relativity with an improvement in sensitivity of over 3 orders of magnitude, improving our understanding of gravity and aiding the developme
Externí odkaz:
http://arxiv.org/abs/0802.0582
Publikováno v:
Publ.Astron.Soc.Jap. 58 (2006) 367-373
We have taken a 4-day spectroscopic observation and have been conducting a 13-day photometric study of the SU UMa-type dwarf nova, ER Ursae Majoris. The mean $K$-amplitude for the emission lines is $54\pm 8$ km s$^{-1}$ and $\gamma$ velocity is 8$\pm
Externí odkaz:
http://arxiv.org/abs/astro-ph/0602181
In this paper we report a new method for determining the thickness of the non-edge-on disk galaxies. Our method is based on the observation comparing with the theoretical researches of the distribution of the vertical velocity dispersion, which is ob
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512390
Publikováno v:
Astron.J.131:1167-1673,2006
We report photometric and spectroscopic observations of the SU UMa-type dwarf novae, KS Ursae Majoris, during its 2003 February superoutburst. Modulations with a period of $0.07017\pm0.00021$ day, which is 3.3% larger than the orbital period, have be
Externí odkaz:
http://arxiv.org/abs/astro-ph/0511468
Publikováno v:
A&A, 1999, 350, 31
This paper presents some statistical correlations of 72 northern spiral galaxies. The results show that early-type spirals that are brighter, and thicker, and the axis ratios ($H_{z}/H_r$) of the disk tend to be smaller along the Hubble sequence. We
Externí odkaz:
http://arxiv.org/abs/astro-ph/0002476
The influence of the outer boundary condition (OBC) on the dynamics and radiation of optically thin accretion flow is investigated. Bremsstrahlung and synchrotron radiations amplified by Comptonization are taken into account and two-temperature plasm
Externí odkaz:
http://arxiv.org/abs/astro-ph/0002068
Publikováno v:
In New Astronomy October 2013 23-24:49-54
Autor:
Peng, Qiuhe qhpeng@nju.edu.cn, Hu, Yiming1, Wang, Kun2, Liang, Yu1, Zha, Jie2, Luo, Zhi-qian2
Publikováno v:
Journal of Astrophysics & Astronomy. Sep2014, Vol. 35 Issue 3, p253-256. 4p. 1 Chart.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.