dc.contributor.editor | Editor of work here. | en_US |
dc.contributor.other | Preservation Department, Stony Brook University Libraries. | en_US |
dc.contributor.other | Cataloging & Metadata Department, Stony Brook University Libraries. | en_US |
dc.date.accessioned | 2007-02-23T21:54:51Z | |
dc.date.accessioned | 2015-04-24T14:41:43Z | |
dc.date.available | 2007-02-23T21:54:51Z | |
dc.date.available | 2015-04-24T14:41:43Z | |
dc.date.issued | 2001-07 | en_US |
dc.identifier.uri | http://hdl.handle.net/1951/36716 | |
dc.identifier.uri | http://hdl.handle.net/11401/69993 | |
dc.description | leave(s) : ill; 28 cm. | en_US |
dc.description | Astronomy Reports -- July 2001
Volume 45, Issue 7, pp. 497-579
Magnetic Fronts in Galaxies
A. P. Petrov, D. D. Sokoloff, and D. L. Moss
pp. 497-501 Full Text: PDF (71 kB)
A Correlation between the Distributions of Pulsars and Emission Measures in the Galaxy
A. V. Pynzar' and V. I. Shishov
pp. 502-509 Full Text: PDF (106 kB)
The Dust Envelope of R Cas
G. Weigelt and B. F. Yudin
pp. 510-516 Full Text: PDF (78 kB)
Wolf���Rayet Stars and Cosmic Gamma-ray Bursts
K. A. Postnov and A. M. Cherepashchuk
pp. 517-526 Full Text: PDF (119 kB)
Observations of Five Supernovae in 1995���1997
D. Yu. Tsvetkov, N. N. Pavlyuk, and E. P. Pavlenko
pp. 527-537 Full Text: PDF (291 kB)
Interpretation of Light Curves of IP Peg in a Model with Shockless Interaction between the Gas Stream and Disk
T. S. Khruzina, A. M. Cherepashchuk, D. V. Bisikalo, A. A. Boyarchuk, and O. A. Kuznetsov
pp. 538-552 Full Text: PDF (281 kB)
Optical Spectra of Three AGB Stars
V. G. Klochkova, G. Zhao, V. E. Panchuk, and N. S. Tavolganskaya
pp. 553-563 Full Text: PDF (126 kB)
A New Approach to Modeling the Surface Magnetic Fields of Chemically Peculiar Stars
V. R. Khalak, Yu. N. Khalak, A. V. Shavrina, and N. S. Polosukhina
pp. 564-568 Full Text: PDF (71 kB)
Convective Mechanism for the Formation of Photospheric Magnetic Fields
A. V. Getling
pp. 569-576 Full Text: PDF (158 kB)
The Hamiltonian in the Planetary or Satellite Problem as a D'Alembertian Function
K. V. Kholshevnikov
pp. 577-579 Full Text: PDF (51 kB) | en |
dc.format | Monograph. | en_US |
dc.format.extent | 1253906 bytes | |
dc.format.extent | 2754 bytes | |
dc.format.medium | Electronic Resource. | en_US |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/html | |
dc.language.iso | en_US | en |
dc.publisher | MAIK ���Nauka/Interperiodica��. | en |
dc.publisher | Stony Brook University. | en_US |
dc.relation.ispartofseries | V. 45 | en |
dc.relation.ispartofseries | I. 07 | en |
dc.rights | All Rights Reserved. Stony Brook University. | en_US |
dc.rights | All Rights Reserved. Stony Brook University. | en_US |
dc.subject | Astronomy Reports | en |
dc.subject.lcsh | Physics | en |
dc.title | Astronomy Reports V. 45, I. 07 | en |
dc.type | Other. | en_US |
dc.description.contributor | The content contained herein is maintained and curated by the Preservation Department. | en_US |
dc.description.contributor | This record is revised and maintained by the content administrators from the Cataloging & Metadata Department. | en_US |
dc.publisher.location | Stony Brook, NY. | en_US |