Zobrazeno 1 - 10
of 20
pro vyhledávání: '"G. S. Shostak"'
Publikováno v:
The Astronomical Journal. 160:162
The Allen Telescope Array was used to search for signals with characteristics similar to the “Wow” signal, the best candidate for an extraterrestrial radio signal found during Ohio State University’s (OSU’s) seven-year 21 cm 10-kHz channel sk
Publikováno v:
Proceedings of the IEEE. 100:1700-1717
The systematic search for extraterrestrial intelligence (SETI) has been ongoing for slightly more than half the century that this journal has been in print, and the topic has been of human interest through recorded history. Are we any closer to detec
Publikováno v:
International Astronomical Union Colloquium. 161:653-656
In June 1995 we used the Parkes 64-m radio telescope to search for narrowband or pulsing signals of extraterrestrial intelligent (ETI) origin from the direction of the galactic center. This strategy was chosen so as to maximize the number of possibly
Autor:
G. S. Shostak
Publikováno v:
International Astronomical Union Colloquium. 161:719-728
A new class of SETI targets is proposed, consisting of stellar systems whose ecliptic planes coincide with our line-of-sight. The most favorable of these systems are moderately separated, edge-on binary stars with at least one solar-type component. S
Autor:
M. T. Bradford, Robert Ackermann, John Ross, Jon Richards, G. S. Shostak, Jill Tarter, Jane Jordan, G. R. Harp, Peter Backus, Samantha Blair, Douglas A. Vakoch, Ken Smolek, Tom Kilsdonk, A. Agrawal
Publikováno v:
SPIE Proceedings.
The 1959 Nature article by Giuseppe Cocconi and Phil Morrison1 provided the theoretical underpinnings for SETI, accompanied in 1960 by Project Ozma2, the first radio search for signals by Frank Drake at the National Radio Astronomy Observatory (NRAO)
Autor:
P. C. van der Kruit, G. S. Shostak
Publikováno v:
Symposium - International Astronomical Union. 100:69-76
Most studies of the mass distribution in spiral galaxies have been based on the observed rotation curves. A serious ambiguity in this approach has always been that the rotation curve contains in itself no information on the mass distribution in the d
Autor:
G. S. Shostak
Publikováno v:
International Astronomical Union Colloquium. 37:489-496
Nous testons l’idée d’Arp à savoir que des groupes multiples de galaxies en intéraction sont éjectés hors de systèmes brillants proches de nous. Les observations à 21 centimètres indiquent que, si ceci est le cas, les membres du groupe en
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 202:21P-24P
Autor:
G. S. Shostak
Publikováno v:
The Milky Way Galaxy ISBN: 9789027719201
The Milky Way Galaxy: Proceedings of the 106th Symposium, Groningen, Netherlands, May 30-June 3, 1983 (A85-46176 22-90), 623-632
ISSUE=106;STARTPAGE=623;ENDPAGE=632;TITLE=The Milky Way Galaxy
The Milky Way Galaxy: Proceedings of the 106th Symposium, Groningen, Netherlands, May 30-June 3, 1983 (A85-46176 22-90), 623-632
ISSUE=106;STARTPAGE=623;ENDPAGE=632;TITLE=The Milky Way Galaxy
It is a decided honor to have the opportunity to address as distinguished a group as is present this evening, and I am particularly grateful for the very complimentary introductory remarks of Harry van der Laan. To paraphrase Einstein's comment on a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f6ce81d4f792bdc63b21ac966394ae5
https://doi.org/10.1007/978-94-009-5291-1_123
https://doi.org/10.1007/978-94-009-5291-1_123
Autor:
E. Brinks, G. S. Shostak
Publikováno v:
Surveys of the Southern Galaxy ISBN: 9789400972193
The Milky Way Galaxy ISBN: 9789027719201
The Milky Way Galaxy ISBN: 9789027719201
The new high resolution HI survey of M31 (Brinks, this volume) was effected at a resolution of Δα × Δδ × ΔV = 24″ × 36″ × 8.2 km s−1. These measures comprise a data cube consisting of 147 channel maps, separated in velocity by 4.1 km s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ecbb505dc8ffd080b9dff2a5796ca920
https://doi.org/10.1007/978-94-009-7217-9_34
https://doi.org/10.1007/978-94-009-7217-9_34