Аккреционные диски. ... C- code to calculate evolution of the accretion disk with time-independent viscosity in a binary system (v0.3 March 2015) ( см. ... Observed flux F=L*Psi(theta)/(4 pi D)^2, where L is the bolometric luminosity, D is the distance to the disk, theta is the angle between the normal to the disk plane and the line of sight, mu = cos(theta), mu=0 when photons go parallel to the disk plane. a=0.0 ; a=0.9981 ; Functions are calculated using different codes: kerrbb ( Li et al., ...

... Authors: D. R. Anderson et al. arxiv:1101.3781 Сверхмассивные черные дыры не коррелируют с галактическими дисками или псевдобалджами (Supermassive black holes do not correlate with galaxy disks or pseudobulges) . ... arxiv:1101.3586 Массивное протоскопление галактик на красном смещении 5.3 (A massive proto-cluster of galaxies at a redshift of z {\approx} 5.3) . Authors: Peter L. Capak et al. arxiv:1101.2022 Первые результаты Планка: проект Планк (Planck Early Results: The Planck mission) . ...

previous next contents elements attributes index . ... Introduction to forms . ... Here's a simple form that includes labels, radio buttons, and push buttons (reset the form or submit it): FORM action= http://somesite.com/prog/adduser method= post P LABEL for= firstname First name : /LABEL INPUT type= text id= firstname BR LABEL for= lastname Last name : /LABEL INPUT type= ... The scope of the name attribute for a control within a FORM element is the FORM element. ...