... All 4 sources show the presence of dust emission, in addition to the synchrotron component; this is also true for M87, for which our aperture includes both the nucleus and the jet. ...
... M 1=2 1 M d [yrs] (4) where 49 = ionizing Lyman continuum ux in units of 10 49 s 1 ... M., Testi, L., Walmsley, C. M., & Olmi, L. 1997, A&A, 325, 725 Cesaroni, R., Felli ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/w75n_sio/w75n_sio.ps.gz -- 503.4 Кб -- 11.09.2007 Похожие документы
... M., Kompe, C., & Churchwell, E. 1991, Ё A&A, 252, 278 Cesaroni, R., Walmsley, C. M ... M., & Cesaroni, R. 1990, A&AS, 83, 119 Churchwell, E., Walmsley, C. M., & Wood, D. O ...
... m dishes that were employed in three different configurations yielding baselines in ... M., Jenness T., Neri R., Olmi L., Robberto M., Testi L., Walmsley C.M., 1999a, A&A ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/g29g31/maxia.ps.gz -- 386.4 Кб -- 11.09.2007 Похожие документы
... m and the offset t of this linear fit, a(DT ) is given by a(DT ) p 1 ( m DT. t ) (5 ... p 8.4 m, D tel p 22.8 m), a commonly used value for L0 of 25 m (Conan et al. 2002 ...
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Ссылки http://www.arcetri.astro.it/~masciadr/PUBLI/egner_masciadri_mckenna_2007.pdf -- 1288.0 Кб -- 21.11.2008 Похожие документы
... M. Baes,4 G. J. Bendo,5 A. Boselli, L. Ciesla,6 M. Clemens,7 E. Corbelli,2 I. De ... m 0.96 1.03 1.03 160 µm 1.06 1.03 0.99 250 µm 1.00 (0.98) 0.99 (0.96) 0.08 (0.94 ...
... measurement (M D 145 M ; ° 3.1) and the estimate of the virial mass (M d D 160 M ... M., Snell, R. L., & Schloerb, F. P. 1990, ApJ, 362, 147 101, 1435 Cesaroni, R ... M., Sargent, A. I., & Churchwell, E. 1998, ApJ, 507, 861 Shepherd, D. S., Yun, K.-C ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/afgl5142_2/afgl5142ovro.pdf.gz -- 431.4 Кб -- 11.09.2007 Похожие документы
... two cores (mmA of 110 M # , and mmB of 11 M # ) embedded in more di#use gas (58 M ... 0.34 (# 2 = 0.42) up to M # 40 M # , with a sig nificantly larger # for M > 40 M ...