Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 81
KRZEMINSKI [ 60 ] has made a plausible estimate of the distance , 8 kpc , using
an assumed absolute magnitude M , = - 5 . 5 mag , an estimated absorption A , =
4 . 4 mag ( based on a ratio of 3 . 2 of total to selective absorption and assumed ...
KRZEMINSKI [ 60 ] has made a plausible estimate of the distance , 8 kpc , using
an assumed absolute magnitude M , = - 5 . 5 mag , an estimated absorption A , =
4 . 4 mag ( based on a ratio of 3 . 2 of total to selective absorption and assumed ...
Page 97
With an assumed intrinsic color B - V = – 0 . 25 , the reddening E ( B – V ) = 0 . 73
and the total visual absorption is about 2 . 2 mag . The infra - red colors out to 3 .
5 um are consistent with interstellar reddening and do not indicate a ...
With an assumed intrinsic color B - V = – 0 . 25 , the reddening E ( B – V ) = 0 . 73
and the total visual absorption is about 2 . 2 mag . The infra - red colors out to 3 .
5 um are consistent with interstellar reddening and do not indicate a ...
Page 170
is assumed . Using the value of vs for aluminum , the most suitable material
readily available in large single ingots with good ... Assuming that the antenna
temperature were low enough for resonator noise to be unimportant , and using o
= 8 .
is assumed . Using the value of vs for aluminum , the most suitable material
readily available in large single ingots with good ... Assuming that the antenna
temperature were low enough for resonator noise to be unimportant , and using o
= 8 .
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Contents
Gruppo fotografico del partecipanti al Corso | 1 |
Introduction | 17 |
Сen | 37 |
Copyright | |
59 other sections not shown
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Common terms and phrases
absorption accretion amplitude analysis angular approximation assumed Astrophys binary black hole calculations charge considered convective core corresponding cycle density dependence detailed detectors determined dips discussed disk distance eclipse effect electromagnetic electron emission energy equation estimate evolution existence expected field Figure flux frequency function geometry give given gravitational important increase indicated intensity interesting Journ less Lett light curve limit lines magnetic mass mean measurements motion Nature neutrino neutron star observed obtained occur optical orbital parameters particle period phase Phys position possible potential present primary pulsations radiation radio range ratio region relation relative rotating scale sensitivity shell shown shows solutions spectrum stellar stellar wind structure suggested surface temperature values variable variations velocity X-ray sources
Bibliographic information
| Title | Proceedings of the International School of Physics "Enrico Fermi.", Volume 65 Proceedings of the International School of Physics "Enrico Fermi.", Società italiana di fisica Rivista del nuovo cimento |
| Contributor | Società italiana di fisica |
| Publisher | N. Zanichelli, 1978 |
| Original from | the University of California |
| Digitized | 14 Aug 2008 |
| ISBN | 0720407206, 9780720407204 |
| Export Citation | BiBTeX EndNote RefMan |