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V.S. Avedisova 《Astrophysics and Space Science》1997,252(1-2):261-272
The main kinematic characteristics of our Galaxy are analyzed using a catalog of about 2700 Galactic star-forming regions. The terminal velocities of the star-forming regions confirm that the rotation curve for the inner Galaxy is flat from |l| 23°. Bends in the rotation curve are probably due to motions in spiral arms. The Galaxy rotates with a circular velocity of 200 ± 10 km s-1. Evidence for an expanding ring-like structure at 3 kpc is presented. An l - v diagram for the catalog sources in the first and fourth Galactic quadrants is constructed. Density wave theory is used to show that a two-spiral model with a pitch angle of -9° and large-amplitude velocity perturbations in the region of 3 kpc can satisfactory describe the main features of the l - v diagram to Galactocentric radii of 6-7 kpc. 相似文献
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A.M. Fridman O.V. Khoruzhii V.V. Lyakhovich V.S. Avedisova O.K. Sil'chenko A.V. Zasov A.S. Rastorguev V.L. Afanas'iev S.N. Dodonov J. Boulesteix 《Astrophysics and Space Science》1997,252(1-2):115-131
General ideas, as well as experimental and theoretical efforts concerning the prediction and discovery of new structures in the disks of spiral galaxies – giant anticyclones - are reviewed. A crucial point is the development of a new method to restore the full vector velocity field of the galactic gas from the line-of-sight velocity field. This method can be used to get self-consistent solutions for the following problems: 1) determination of non-circular velocities associated with spiral-vortex structure; 2) determination of fundamental parameters of this structure: pattern speed, corotation radius, location of giant anticyclones; 3) refinement of galactic rotation curves taking into account regular non-circular motion in the spiral density wave, which makes it possible to build more accurate models of the mass distribution in the galaxy; 4) refinement of parameters of the rotating gaseous disk: inclination angle, center of rotation and position angle of the major dynamical axis, systematic velocity. The method is demonstrated using the restoration of the velocity field of the galaxy NGC 157 as an example. Results for this and some other spiral galaxies suggest that giant anticyclones are a universal property of galaxies with grand design structure. 相似文献
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GeoJournal - Systems' ideas are organically inherent in the integrational potential of geography. Analysis of evolution of understanding of a “geosystem” witnesses for ecologization... 相似文献
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V. S. Avedisova 《Astronomy Reports》2002,46(3):193-205
This Catalog of Star-Forming Regions in the Galaxy contains coordinates and fluxes of young objects in the radio and infrared, as well as data on the radial velocities of recombination and molecular lines, for more than three thousand star-forming regions. In addition to photometric and kinematic data, we present information on diffuse and reflecting nebulae, dark and molecular clouds, and other objects related to young stars. The catalog consists of two parts. The main catalog lists star-forming regions in order of Galactic longitude and is supplemented by analogous information for star-forming regions in complexes of dark clouds with large angular sizes that are closest to the Sun. The main catalog is located at http://www.strasbg.-u.fr/pub/cats. In our preliminary study of the catalog data using a formal classification of the star-forming regions, we subdivided these objects into several classes and characterized them as being populated primarily by massive or low-mass stars at early or late stages of the star-formation process. We also distinguish between relatively nearby and distant complexes. 相似文献
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V. S. Avedisova 《Astronomy Reports》2005,49(6):435-445
We obtained the photometric distances and radial velocities for the molecular gas for 270 star-forming regions and estimated the distance to the Galactic center from ten tangent points to be R0 = 8.01 ± 0.44 kpc. Estimates of R0 derived over the last decade are summarized and discussed; the average value is R0 = 7.80 ± 0.33 kpc. We analyze deviations from axial symmetry of the gas motion around the Galactic center in the solar neighborhood. Assuming a flat rotation curve, we obtain Θ0 ~ 200 km/s for the circular velocity of the Sun from regions beyond the Perseus arm. We used these Galactic constants to construct the Galactic rotation curve. This rotation curve is flat along virtually its total extent from the central bar to the periphery. The velocity jump in the corotation region of the central bar in the first quadrant is 20 km/s. We present analytical formulas for the rotation curves of the Northern and Southern hemispheres of the Galaxy for R0 = 8.0 kpc and Θ0 = 200 km/s. 相似文献
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