... to 5m. The smaller eclipse depth that is observed at longer wavelengths has been attributed to thermal radiation from the secondary with a color temperature of 500 K (Backman et al. ...
... 2 4 -2 5 , 2 0 1 0 An e ta Si e m i g i n o wska , CfA Small Challenges · CHASC ... 2 4 -2 5 , 2 0 1 0 An e ta Si e m i g i n o wska , CfA Past Challenges 1997 Meeting ... 2 4 -2 5 , 2 0 1 0 An e ta Si e m i g i n o wska , CfA Current Challenges ...
[
Текст
]
Ссылки http://hea-www.harvard.edu/AstroStat/CAS2010/asiemiginowska_CAS2010aug24.pdf -- 126.8 Кб -- 26.08.2010 Похожие документы
... and J. McCarthy, University College, Cork, report: "Photometric and spectroscopic observations of CI Cam, the possible counterpart of XTE J0421+56 (IAUC 6855, 6857), were obtained with the 1.2-m and 1.5-m telescopes at the Whipple Observatory during Apr ...
... 27.1 UT with the 1.5-m telescope (+ FAST spectrograph) of the F. L. Whipple Observatory at Mt. Hopkins, using the position reported by Israel et al.. ...
... 2 R. A. Cameron, G. Hasinger,1 B. T. Jannuzi,5M. G. Smith,6 P. S. Smith,7 and H ... available through NOAO (i.e., WIYN / 3.5m, Blanco 4 m, Gemini-N ) and SAO (i.e ...
[
Текст
]
Ссылки http://hea-www.harvard.edu/~kim/pap/2008_ChaMP_AGN_XLF.pdf -- 1611.9 Кб -- 06.12.2010 Похожие документы
... Throughout, we assume the following cosmological parameters for distance-dependent 5 quantities: m = 0.3, = 0.7, and H0 = 72 km s-1 Mpc-1 . 2. ...
[
Текст
]
Ссылки http://hea-www.harvard.edu/~pgreen/BIQSOS/ChandraBiQSOs4.pdf -- 472.9 Кб -- 24.03.2011 Похожие документы
... In addition, a model disk optically thick enough to reproduce the mid-eclipse brightening in single-color data would only produce a ``gray'' eclipse if virtually all the particles in the disk are much larger than 5m in radius. ...