... near-diffraction limited imaging spectroscopy in the 0.94-2.5 m m wavelength range ... SpT . P max . (%) . l max . ( m m) . P.A. (deg) . K . (mag) . ... Wavelength ( m m) . Identification . Wavelength ( m m) . Identification . ...
35. http://www.mso.anu.edu.au/~charley/papers/JonesLineweaver2010.pdf
... m of the solute is given by Raoult's equation: DTb ј Kb m, where Kb is the ... Amato, P., Menager, M., Sancelme, M., Laj, P., Mailhot, G., and Delort, A. (2005 ... M., Fredrickson, J., Keefe, A., Keller, M., McSween, H., Nealson, K., Sherwood ...
36. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Bizyaev04
... that Mt ј Ms Ч Md and LB ј Md =(M =L), where M/L denotes the B-band stellar mass-to ... M s =M d ю M b =M d ј : Md Ч Mb 1 Ч M b =M d П 1ч The values of Mb =Md can be ...
37. http://www.mso.anu.edu.au/~geoff/HEA/4_Synchrotron_Radiation_II.pdf
... Synchrotron Radiation II 81/93 and 2 me 2 p = ----------- -------- = ----------- ----------- 0 -2 a + 1 2 0 a + 1 e2 0 4 B2 then a+5 2 ----------me 1 e 2 1 2 2 ----------- ----------- ------------ 0 = 1 + c E C 2 1 a ------- a + 1 e2 m c2 0 c 0 e I ...
38. http://www.mso.anu.edu.au/~gdc/prepr/AndII_vars.pdf
... 106, 250 Zinn, R., & West, M. J. 1984, ApJS, 55, 45 TA P BLE 1 H OT O M E T R I C D I FF E R E N C E S Chip Note. -- difference ...
39. Untitled
... Observatory with Jim Liebert during 1979, showed these stars to be exotic M subdwarfs (paper 58*) and very cool M dwarfs ... star, the bright M subdwarf, had a metallicity of about -0.7 dex while the abundance of VB 12, the faint M subdwarf companion ...
40. http://www.mso.anu.edu.au/~geoff/HEA/Wilson_Cygnus_A.pdf
... M. 1974, MNRAS, 166, 305 Harris, D. E., Carilli, C. L. & Perley, R. A. 1994, Nature, 367, 713 (HCP) Harris, D. E., Leighly, K ...