凝乳
发表于 2025-3-25 04:49:10
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
自由职业者
发表于 2025-3-25 08:58:05
http://reply.papertrans.cn/19/1802/180175/180175_22.png
夹死提手势
发表于 2025-3-25 14:19:11
http://reply.papertrans.cn/19/1802/180175/180175_23.png
GRIEF
发表于 2025-3-25 18:45:36
http://reply.papertrans.cn/19/1802/180175/180175_24.png
雪崩
发表于 2025-3-25 22:28:46
http://reply.papertrans.cn/19/1802/180175/180175_25.png
Parabola
发表于 2025-3-26 01:32:03
http://reply.papertrans.cn/19/1802/180175/180175_26.png
Afflict
发表于 2025-3-26 07:49:10
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
发表于 2025-3-26 09:05:47
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
发表于 2025-3-26 15:49:30
Handbook of Precision Engineeringand 19381+2224 respectively by Dong & Hu (1991) among other sources having very strong infrared excesses, V- > 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
发表于 2025-3-26 18:55:26
http://reply.papertrans.cn/19/1802/180175/180175_30.png