Titlebook: B[e] Stars; Anne Marie Hubert,Carlos Jaschek Book 1998 Springer Science+Business Media B.V. 1998 Galaxy.LOPES.galaxies.interferometry.phot

凝乳

Automated Staining: Dako Perspective,han .. =11.5 mag (ESA 1997, ESA SP-1200) . These two filters are roughly centered on the B and V Johnson filters. A simple linear transformation exists between Tycho .. and . magnitudes and B and V magnitudes in the Johnson photometric system (see ESA 1997) . The Tycho Epoch Photometry Annex A conta

自由職業(yè)者

夾死提手勢(shì)

GRIEF

雪崩

Parabola

Afflict

Handbook of Precision Engineeringtellar envelopes around peculiar Ae/Be stars. The method involved is based on a search for rapid line-profile variability of lines originating in different circumstellar regions. Analysis of these variations opens the way for reconstructing the density and velocity distributions throughout the envel

尾巴

Electrical and Electromagnetic Components, al., 1992; Araújo and Freitas Pacheco, 1994). These stars share several common characteristics as an optical spectra dominated by Balmer and FeII emission lines (often displaying P Cygni profiles) and absorption lines of FeII and other low ionization species in the UV. Besides, prominent emissions

CAGE

Handbook of Precision Engineeringand 19381+2224 respectively by Dong & Hu (1991) among other sources having very strong infrared excesses, V-[25] > 8. . Only one . photometric observation has been published (Haug 1970) for AS 78 which was discovered by Miller & Merrill (1951) as a Be star. A spectral type of B9 I a or B2–5 v was es

吞噬