On the Form of the Distribution Law of Stellar Velocities.
نویسنده
چکیده
Legends for Fig. 2 IV. so Persei. This star is not known to be a variable. The observations are of moderate accuracy, being normal places from one-prism observations by Jordan at Allegheny. It is a star of very complex and erratic behavior. Cannon5 (observations not shown) postulated a secondary of one-half the main period, but it is impossible to satisfy Jordan's data in this manner. V. 62 Cygni.6 Not known to be a variable. The observations are of moderate accuracy, being normal places from one-prism observations by Cannon at Ottawa, with the inclusion of four Lick three-prism values. The observations are grouped almost precisely as would be expected were there a blend effect, but such an effect was searched for without result. Cannon's primary has vn eccentricity of 0.18, and he introduces a secondary of one-third the main period. I cannot satisfy these observations with a single hump, as in the cases given before. It is of interest to see that an entirely different orbit from that of Cannon shows some measure of agreement. More observations are urgently needed on this star, particularly just after maximum velocity of recession, to decide on the character and reality of its deviations. VI. ,B Cephei.7 A Cepheid variable of unusually short period 0d.19 Crump's observations with the Detroit Observatory one-prism are normal places and of rather high accuracy. My curve does not satisfy these places quite so well as does his orbit, which postulates a secondary of one-third the main period, with a semi-amplitude of but 1.25 km. One purpose of this paper will be fulfilled if those possessing instruments of adequate power will accumulate many more observations of the light and velocity curves of the Cepheids; only with such assistance will it ever be possible to solve the many puzzles which they present. 1 Campbell, Astrophys. J., 13, 1900 (90). 2 Curtiss, Lick Obs. Bull.,.3, 1904 (62). 3Plaskett, Publ. Dom. Obs., 2, No. 2, 1915. 4Jordan, Publ. Allegh. Obs., 3, 1913 (31). 5Cannon, J. R. A. S. Canada, 4, 1910 (195). 6 Cannon, Astrophys. J., 47, 1918 (193). 7 Cramp, Pubi. Detroit Obs., 2, 1915 (144). 8 Dncan, Lick Obs. Bull., 5, 1908 (82).
منابع مشابه
The effect of variation of stellar dispersion velocities by the galactic latitude in interpreting gravitational microlensing observations
Our galaxy is a spiral galaxy and its stars are mostly in a thin disk and rotate around the galactic center. The vertical component of the dispersion velocity of stars is a function of the galactic latitude and decreases with increasing it. In the galactic Besancon model, this dependence is ignored and they just consider the dependence of dispersion velocity on the stellar age. Becanson model i...
متن کاملRelativistic Stellar Models with Quadratic Equation of State
In this paper, we have obtained and presented new relativistic stellar configurations considering an anisotropic fluid distribution with a charge distribution and a gravitational potential Z(x) that depends on an adjustable parameter. The quadratic equation of state based on Feroze and Siddiqui viewpoint is used for the matter distribution. The new solutions can be written in terms of elementar...
متن کاملOn Static Bending, Elastic Buckling and Free Vibration Analysis of Symmetric Functionally Graded Sandwich Beams
This article presents Navier type closed-form solutions for static bending, elastic buckling and free vibration analysis of symmetric functionally graded (FG) sandwich beams using a hyperbolic shear deformation theory. The beam has FG skins and isotropic core. Material properties of FG skins are varied through the thickness according to the power law distribution. The present theory accounts fo...
متن کاملThe Geometry of Karbandi in Persian Architecture; Response to the Challenges of Conventional and Stellar Karbandi
Karbandi is one of the original and ancient arched elements in Persian architecture which is formed based on a network with harmonic geometry and in addition to architectural function, it also has structural behavior. However, there are ambiguities about the geometry of this architectural element that should be addressed with targeted research. One of these ambiguities is to determine how the g...
متن کاملStellar Populations in the Central Galaxies of Fossil Groups
It is inferred from the symmetrical and luminous X-ray emission of fossil groups that they are mature, relaxed galaxy systems. Cosmological simulations and observations focusing on their dark halo and inter-galactic medium properties confirm their early formation. Recent photometric observations suggest that, unlike the majority of non-fossil brightest group galaxies (BGGs), the central early-t...
متن کاملBuckling Behaviors of Symmetric and Antisymmetric Functionally Graded Beams
The present study investigates buckling characteristics of both nonlinear symmetric power and sigmoid functionally graded (FG) beams. The volume fractions of metal and ceramic are assumed to be distributed through a beam thickness by the sigmoid-law distribution (S-FGM), and the symmetric power function (SP-FGM). These functions have smooth variation of properties across the boundary rather tha...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
- Proceedings of the National Academy of Sciences of the United States of America
دوره 9 6 شماره
صفحات -
تاریخ انتشار 2005