... molecular component of G24.78 (here after indicated as G24.78+0.08M) are presented: this cor responds to the ammonia emission associated with the wa ter maser spots in the G24.78 region at ff ' 18 h 33 m31 s and ffi ' \Gamma7 ffi 14 0 40 00 (see Sect ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/nh3_ctc/vla.ps.gz -- 541.2 Кб -- 11.09.2007 Похожие документы
... Also included in Fig. 3a (light blue stars) are the IRAS 100 m data, i.e. the LF for all VCC galaxies in the field with an IRAS 100 m detection (31 galaxies). ...
... on 0 , and its first moment (frequency offset) are given by: 3B /2 a(0 ) = -B /2 A(, nu0 )d 1 a± 3B /2 -B /2 (31) (32) m(0 ) = ( - 0 )A(, 0 ))d Both quantites must be computed separately for the real and imaginary parts of the signal, using A r and Ai ...
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Ссылки http://www.arcetri.astro.it/science/Radio/alma/ALMA_Memo_583.pdf -- 260.2 Кб -- 25.02.2010 Похожие документы
... center ff(J2000)=18 h 06 m 14.88 s ffi(J2000)=\Gamma20 ffi 31 0 40.8 00 Parameter 3 ... F2:0cm F1:3cm F0:7cm 18 h 06 m \Gamma20 ffi 31 0 (mJy) (mJy) (mJy) (mJy) F 14. s 884 ...
... continuum emission: 2900 M fi for G29.96\Gamma0.02 and 1500 M fi for G31.41+0.31 ... we obtained a mass of 1600 M fi for G29.96\Gamma0.02 and 3200 M fi for G31.41+0.31 ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/g29g31/maxia.ps.gz -- 386.4 Кб -- 11.09.2007 Похожие документы