... L = 4 nHV + E (1) stellar population of age t with our star formation history: t L (t ) = 0 (t ) 106 M L SSP (t - t ) dt ... SFHs, modelled by convolving the luminosity, LSSP (t ), of a 106 M single (a)]C gra ,abs (a), (15) where the weighting ...
6. http://www.mrao.cam.ac.uk/~bn204/publications/2015/1503.02650v2.pdf
... University of Arizona Press, 524 Brown, R. H., Morrison, D., Telesco, C. M., & Brunk, W. E. 1982, Icarus, 52, 188 Bus, S. J., & Binzel, R. P. 2002, Icarus, 158, 106 Busch, M. W. 2009, Icarus, 200, 347 Campbell, M. J., & Ulrichs, J. 1969, J. Geophys ...
7. http://www.mrao.cam.ac.uk/ppeuc/hep/ward/ward.ps
... Mass peak in \SigmaM = M ij +M kl at ё 106 GeV. ffl ALEPH sees (smaller) peak at same mass at 161 and 172 GeV Other experiments see nothing 0 5 10 15 20 25 30 35 20 40 60 80 100 120 140 160 180 200 SM for minimum dM events/4 GeV N exp =87.6 N data =90 0 2 ...
8. G33.2-0.6
... ADS . Reich 1982, A&A, 106, 314. Effelsberg 100-m at 2.7 GHz (4'.4: S=2.6?0.3 Jy) and 4.75 GHz (2'.5: S=1.75?0.2 Jy). ADS . ...
9. G33.2-0.6
... ADS . Reich 1982, A&A, 106, 314. Effelsberg 100-m at 2.7 GHz (4'.4: S=2.6?0.3 Jy) and 4.75 GHz (2'.5: S=1.75?0.2 Jy). ADS . ...
10. G33.2-0.6
... ADS . Reich 1982, A&A, 106, 314. Effelsberg 100-m at 2.7 GHz (4'.4: S=2.6?0.3 Jy) and 4.75 GHz (2'.5: S=1.75?0.2 Jy). ADS . ...