... If the torus consists of clouds of dust, each with a relatively unobscured view of the higher energy photons from nearer the center of the AGN, the temperature of each dust cloud will fall off as roughly the inverse square root of the radius. ...
... S8 : Interstellar dust and gas coupling: linking observations, models and laboratory astrophysics . S9 : The Dynamics of Star and Planet Formation . ...
... EH And IR excess. The presence of a dust envelope is possible. EO And Very red. ... I = 0.55P. EY And I - K = 5.38; the presence of a dust envelope is possible [06947 ... Surrounded with a dust envelope [08029]. KX And SB2 (P = 38.908d). ...
... Bq [] star with the excess of infrared radiation of dust at T = 300degK. ... Very large IR exess due to expanding gaseous-dust envelope. ... mkm) have a secondary maximum (JD2443815) due to the formation of the dust envelope ...
... the Mg ii 2800 ° A doublet flux and equivalent width variability is much less than the stellar rotation period, which means that the variability is the result of some non-stationary process rather than rotational modulation or occultation by dust clouds ...
... EH And IR excess. The presence of a dust envelope is possible. EO And Very red. ... I = 0.55P. EY And I - K = 5.38; the presence of a dust envelope is possible [06947 ... Surrounded with a dust envelope [08029]. KX And SB2 (P = 38.908d). ...