排序方式： 共有34条查询结果，搜索用时 15 毫秒
31.
V. L. Afanas’ev S. N. Dodonov A. V. Moiseev O. V. Verkhodanov A. I. Kopylov Yu. N. Pariiskii N. S. Soboleva A. V. Temirova O. P. Zhelenkova W. M. Goss 《Astronomy Reports》2003,47(5):377-385
The results of spectroscopic observations of the host galaxies of objects in the RC catalog (the “Big Trio” program) obtained using the new SCORPIO spectrograph of the Special Astrophysical Observatory are presented. The spectroscopic redshifts of the objects are compared with their photometric color redshifts, and the errors in the latter are estimated. Based on BV RI observations obtained on the 6-m telescope of the SAO, the errors for the population of powerful radio galaxies are close to those found previously for radio quiet galaxies (about 10–20%). The detection of Ly α in the B filter in RC 1626+0448 is confirmed. This object is the second spectrally studied FR II radio source from the RC catalog to have a redshift z>2.5. Star formation in its host galaxy began at a redshift z>3.3. This first use of the new SCORPIO spectrograph demonstrates its promise for studies of very distant steep-spectrum radio galaxies brighter than 23m–24m in V. 相似文献
32.
V. N. Koneshov V. B. Nepoklonov V. V. Pogorelov V. N. Solov’ev L. V. Afanas’eva 《Izvestiya Physics of the Solid Earth》2016,52(3):443-451
The application of the airborne gravimetry method for gravity measurements in the Arctic is considered. This method has been extensively employed in foreign studies for determining the figure of the Earth in high-latitude conditions. The possibility of conducting comparative studies along the extensive survey lines and the necessity of aerogravimetry studies for improving the global Earth’s gravity field (EGF) models are discussed. The possibility of the efficient application of the modern EGF models for estimating the systematical errors for different types of gravimetry surveys and exploring the influence of the anomalous far-zone field in the calculations of the plumb line deviations is demonstrated. 相似文献
33.
The formation history of dispersion halos of kimberlite indicator minerals in the Siberian Platform is described beginning from the main Middle Paleozoic productive epoch of kimberlite magmatism. The history and formation conditions of the halos are reconstructed from the ontogeny and typomorphism of indicator mineral assemblages with involvement of the geological history of the Siberian Platform. The general trend characterizing the development of indicator mineral halos is discussed. The data obtained allow adequate estimation of of the character and geological setting of indicator mineral halos for forecasting purposes. 相似文献
34.
Observations of the nebula associated with the WO star in the galaxy IC 1613 are presented. The observations were carried out with a scanning Fabry-Perot interferometer in Hα using the 6-m Special Astrophysical Observatory telescope; narrow-band Hα and [O III]images were obtained with the 4-m KPNO telescope (USA). The monochromatic Hα image clearly reveals a giant bipolar shell structure outside the bright nebula S3. The sizes of the southeastern and northwestern shells are 112×77 and (186–192)×(214–224) pc, respectively. We have studied the object’s kinematics for the first time and found evidence for expansion of both shells. The expansion velocities of the southeastern and northwestern shells exceed 50 and 70 km s?1, respectively. We revealed a filamentary structure of the shells and several compact features in the S3 core. A scenario is proposed for the formation of the giant bipolar structure by the stellar wind from the central WO star located at the boundary of a “supercavity” in the galaxy’s H I distribution. 相似文献