Zobrazeno 1 - 10
of 50
pro vyhledávání: '"Glownia, J. H."'
Autor:
Sorokin, P. P., Glownia, J. H.
A conceptually novel model - one in which stimulated (i.e. induced) resonance Rayleigh scattering causes ions of select species to become accelerated to very high terminal velocities in the solar winds of OB-type stars - is proposed to explain the ge
Externí odkaz:
http://arxiv.org/abs/astro-ph/0410465
Autor:
Sorokin, P. P., Glownia, J. H.
A model is suggested to explain the frequently observed presence of intense, narrow-band, H(alpha) emission lines in the optical spectra of reddened, early-type stars (e.g. HD 44179, IRAS 18179-1346, IRAS 20298+4011). It is proposed that hydrogen ato
Externí odkaz:
http://arxiv.org/abs/astro-ph/0106445
It is shown that, under sufficiently intense OB-star illumination of a stationary photoexcitation front (PDR), nonlinear H2 photoexcitation processes comprising driven resonant two-photon transitions between X-state quantum levels, with VUV continuum
Externí odkaz:
http://arxiv.org/abs/astro-ph/0011396
Publikováno v:
Journal of Chemical Physics; 8/1/1993, Vol. 99 Issue 3, p1654, 10p, 9 Graphs
Publikováno v:
Journal of Chemical Physics; 3/1/1991, Vol. 94 Issue 5, p3389, 18p
Publikováno v:
Journal of Chemical Physics; 3/15/1990, Vol. 92 Issue 6, p3335, 5p
Publikováno v:
Journal of Chemical Physics; 5/1/1985, Vol. 82 Issue 9, p4086, 16p
Publikováno v:
Applied Physics B: Lasers & Optics. 1996, Vol. 63 Issue 5, p421. 4p.
Publikováno v:
Supercontinuum Laser Source; 2016, p299-336, 38p
Publikováno v:
Proceedings of SPIE; Nov2006 Part 2, Issue 1, p62612Q-62612Q-9, 9p