... 1 kpc distance of the SNR, the molecularclouds, or parts thereof could be located ... rays interacting with the dense molecularclouds in this region; the resulting gamma ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/E10_Hofmann01_04Jan07_11:09:00.pdf -- 1695.6 Кб -- 07.11.2006 Похожие документы
... hydrogen gas in the nuclear bulge is trapped in small high density molecularclouds ... Penetration of cosmic rays into molecularclouds was analyzed in a number of papers ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/A06_Dogiel01-05Apr07_00:55:03.pdf -- 130.8 Кб -- 04.04.2007 Похожие документы
... the two-flow jet from the active galactic nucleus and the intergalactic medium Quasar partial coverage effect for intervening molecularclouds On the Statistical Theory of Spatial Structure Formation in Random Media Radio Halos in ACT SZ-selected Galaxy ...
... in a circumstellar cloud [34]: the bolometric light curves for the afterglow resulting from the passage of the blast wave through a molecularcloud were computed, implying that the peak of the emission could be reached as soon as seven days (the gamma-ray ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/I06_Castro-Tirado01-16May07_19:00:26.pdf -- 582.1 Кб -- 16.05.2007 Похожие документы
... We present also arguments that protons from Sgr A may also produce a flux 6.4 keV line and bremsstrahlung continuum emission from molecularcloudsclouds. ...
... Another possible application is the three-dimensional location of the bright sources with respect to the numerous giant molecularclouds in this region. ...
... With a model for the rate of low-mass star formation in molecularclouds McKee [6] finds a SFR of 3.6 M /yr from the analysis of thermal radio emission from HII regions, which is proportional to the production rate of ionizing photons, which in turn is ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B07_Hartmann01-07May07_12:04:00.pdf -- 279.4 Кб -- 07.05.2007 Похожие документы
... The nuclear bulge (NB) of the Galaxy appears as a massive disk-like complex of stars and molecularclouds of radius ~250 pc and height ~50 pc, located in the Galactic center region, and which is distinct from the Galactic bulge, as described in Launhard ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B34_Schanne03-23Jan07_09:40:00_bandw.pdf -- 234.9 Кб -- 24.01.2007 Похожие документы
... The aim of the present work is to detect for the first time the transient sources embedded in this dense molecularcloud, as well as those fainter persistent supergiant ones. ...