[4] viXra:1107.0051 [pdf] submitted on 24 Jul 2011
Authors: Alon Retter
Comments: 4 pages
It is a known fact that like people, many stars are single while most others tend to couple in
binaries, yet the two distributions have not been compared so far. The distribution of 4559
brightest nearby stars was matched with that of American adults at the age of 18-65 years. It
was found that the mean values of the distributions of star multiples and US households are
almost identical (2.04 vs. 2.03). Moreover, a strong resemblance between the two curves is
evident. Monte Carlo simulations suggest that this result is significant at a confidence level
higher than 97%. Apparently, there should be no connection between the two populations,
thus this striking result may supply some clues about the way Nature works.
Category: Astrophysics
[3] viXra:1107.0013 [pdf] submitted on 5 Jul 2011
Authors: Jin He
Comments: 12 Pages
Weakly interacted galaxies present very simple body structure. They are
either three-dimensional objects resembling ellipsoids or flat-shaped disks showing spiral
disturbance. Elliptical galaxies present little dust and gas but spiral galaxies demonstrate
arms and rings which are characterized by containing a huge amount of dust and gas. Since
arms and rings are linear-shaped, the body structure of spiral galaxies may be a textured one
as earth-bound materials always are. This led to the concept of rational structure which is
based on proportion curves. The proportion curves for normal spiral galaxies are all equiangular
spirals which trace or cut through arms consistently. This paper demonstrates the
spider-shaped proportion curves for barred spiral galaxies. It shows for the seventh galaxy
(NGC 5921) that the curves do trace or cut through arms or rings consistently. More examples
of barred galaxies will be studied for the testification of Nature�s rationality.
Category: Astrophysics
[2] viXra:1107.0012 [pdf] submitted on 5 Jul 2011
Authors: Jin He
Comments: 12 Pages
Weakly interacted galaxies present very simple body structure. They are
either three-dimensional objects resembling ellipsoids or flat-shaped disks showing spiral
disturbance. Elliptical galaxies present little dust and gas but spiral galaxies demonstrate
arms and rings which are characterized by containing a huge amount of dust and gas. Since
arms and rings are linear-shaped, the body structure of spiral galaxies may be a textured
one as earth-bound materials always are. This led to the concept of rational structure which
is based on proportion curves. The proportion curves for normal spiral galaxies are all
equiangular spirals which trace or cut through arms consistently. This paper demonstrates
the spider-shaped proportion curves for barred spiral galaxies. It shows for the sixth galaxy
(NGC 5701) that the curves do trace or cut through arms or rings consistently. More examples
of barred galaxies will be studied for the testification of Nature�s rationality.
Category: Astrophysics
[1] viXra:1107.0011 [pdf] submitted on 5 Jul 2011
Authors: Jin He
Comments: 12 Pages
Weakly interacted galaxies present very simple body structure. They are
either three-dimensional objects resembling ellipsoids or flat-shaped disks showing spiral
disturbance. Elliptical galaxies present little dust and gas but spiral galaxies demonstrate
arms and rings which are characterized by containing a huge amount of dust and gas. Since
arms and rings are linear-shaped, the body structure of spiral galaxies may be a textured
one as earth-bound materials always are. This led to the concept of rational structure which
is based on proportion curves. The proportion curves for normal spiral galaxies are all
equiangular spirals which trace or cut through arms consistently. This paper demonstrates
the spider-shaped proportion curves for barred spiral galaxies. It shows for the fifth galaxy
(NGC 4930) that the curves do trace or cut through arms or rings consistently. More examples
of barred galaxies will be studied for the testification of Nature�s rationality.
Category: Astrophysics