... consists of star-formation driven thermal opacity and supernova-driven synchrotron component Prior : 0.5 kpc comp: -1 < < -1/2, 10-1 yr-1 < SN rate < 101 1 M yr-1 < SFR < 103 M yr-1 , 10-3 < areal filling factor 0.05 kpc comp: -1 < < -1/2, 10-1 yr-1 < SN ...
5. References
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6. Abstract
... G. Ventura, G. Dall'Oglio, L. Pizzo, R. Cosimi, A. Miriametro, L. Martinis, L. Piccirillo, M. Bersanelli, and G. Morgante ... TESRE, Consiglio Nazionale delle Ricerche, Via Gobetti 101, 40129 Bologna, Italy . Dip. ...
7. Abstract
... For this paper: postscript PPEUC CMB index 1 Introduction... N. Mandolesi, M. Seiffert, M. Bersanelli, and C. Burigana . ... Istituto TESRE, Consiglio Nazionale delle Ricerche, Via Gobetti 101, 40129 Bologna, Italy . ...
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9. G17.8-2.6
... References: . Reich et al. 1988, IAUCo, 101, 293. Summary of parameters. ADS . ... 1990, A&AS, 85, 633. Effelsberg 100-m at 2.7 GHz (4'.3). ADS . Green et al. ... Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations. ADS . Sun et al. ...
10. Abstract
... C. Burigana, D. Maino, N. Mandolesi, E. Pierpaoli, . M. Bersanelli, L. Danese, and M.R. Attolini . ... Istituto TESRE, Consiglio Nazionale delle Ricerche, Via Gobetti 101, 40129 Bologna, Italy . ...