... 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. ...
... C.M. Walmsley1 , R. Cesaroni1 , C. Codella1 , F. Schuller2 L. Bronfman3 , S.J ... 1) luminosity drops with Lbol /M , which suggests that jet activity declines as time ...
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Ссылки http://www.arcetri.astro.it/science/starform/preprints/sepulcre_03.pdf -- 938.6 Кб -- 24.11.2010 Похожие документы
... m- M mag <0.97 32.17 0.11 32.53 <0.16 32.49 <0.20 32.60 0.86 32.73 0.16 32.66 1 ... M. A., Sutherland, R. S., Heisler, C. A., & Trevena, J. 2001, ApJ, 556, 121 Khochfar ...
... M. Boer,3 C. Clemens,11 F. D'Alessio,9 16,17,18 M. Della Valle, S. di Serego ... jet with a bright narrow core and fainter wings can also produce a rebrightening ... M., 2007, ApJ, 667, 340 Starling R. L. C., Wijers R. A. M. J., Wiersema K., Rol E ...
... transferred to the ambient gas (n H2 m H2 V 2 ), by R2 , under ... the water masers tracing the jet in G28.87+0.07, we use all the ... We note that the derived parameters for the jet in G28.87+0.07 ...
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Ссылки http://www.arcetri.astro.it/science/starform/preprints/mosca_06.pdf -- 1253.0 Кб -- 17.01.2012 Похожие документы
... jet of relativistic electrons the magnetic field should be perpendicular to the lo ... M. C. Begelman, R. D. Blandford and M. J. Rees, Rev. Mod. Phys. 56 (1984) 255. ... H. D. Tran, M. H. Cohen, P. M. Ogle, R. W. Goodrich and S. di Serego Alighieri ...
... optics [MCAO] vM [where M is the number of the deformable mirrors, with M p 1, 2, 3 ... jet-stream region (1015 km; Fig. 10, solid line) is equal to 10 15 k m p 0 .22 ...
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Ссылки http://www.arcetri.astro.it/~masciadr/PUBLI/masciadri_egner_2006.pdf -- 718.0 Кб -- 21.11.2008 Похожие документы
... M., Bettarini, A., Catarzi, M., Curioni, G.P., Curioni, P., Di Franco, S ... M., Palla, F. : 2003, invited review in Asteroseismology across the HR diagram, eds ... M., Bernabei, S., Palla, F., Pinheiro, F.J.G., Folha, D.F.M., Oswalt, T.D ...
... M d ё 145 M fi , Sect. 3.1), and the estimate of the virial mass (M vir ё 160 M fi ... J.M., Snell, R.L. & Schloerb, F.P. 1990, ApJ, 362, 147 Cesaroni, R., Felli, M ... C.M. 1998, A&A, 329, L33 -- 15 -- Lekht, E.E., Marquez, A. & Mendozatorres, J.E ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/afgl5142_2/afgl5142ovro.ps.gz -- 339.4 Кб -- 11.09.2007 Похожие документы