the celestial objects with high redshift (quasar, qso) are often blue and punctiform
You find below the explanation of some of the used terms:
- M.y.l . is the distance covered by the ligth in one million of years;
- anom. vel. is a not-existing movement (because measured with Doppler effect);
- Doppler effect is the effect of the movement over the received wave;
- rad. vel. is the movement considered perpendicolarly to the observer in km/s. per y.l.;
- redshift is the rad. vel. in relation to the ligth speed;
- accel. is the increase of speed in cm/sec per sec;
- tot. anom. incr. is the total false increase of vel. in the true distance in y.l.;
- true dist. is the presumption of the amateur;
- rad. temp. is the average temperature of the departing waves;
- k2 is related to the effects of the gradient of plasma, of gravitation, of ionic
ejection ...(some of the components of k2 could enter as a factor in the main
formula)
- the celestial objects with high redshift (quasar, qso) are often blue and point sourced :
from the book libro "Fisica senza dogma" - Franco Selleri (Edizioni Dedalo, pag. 211), we learn that the celestial objects with high redshift are often point sourced (big distance ), blue (higth temperature) and source of radio waves (high activity);
therefore the redshift can have relation with distance, temperature and activity...
- the warmer a stars is, the higher his rad.vel. is (rad.vel is proportional to the star temperature) :
In order to prove this sentence we should consider 2 groups of stars with known distance, having different values of temperature, and compare the averages of their rad. vel. The proposed formula for the effects of the temperature over the rad. vel., shows that the stars with 24000 degrees of temperature and distant from us 1000 y.l., have the rad. vel. anormally increased of: rad.vel. =25*1000/1000 000 *5^3 ≈ 3 km/s; this quantity is detectable only having a great and homogeneous number of data.
We shall come back later on that demonstration but now, more easily, we just use a catalogue (downloadable from http://csdweb.u-strasbg.fr/viz-bin/Cat?III/210), who contains the data of 4000 white dwarf stars (The dwarfs have higth temp. and elevate k2 ). In this catalogue there are only 80 starts that have both the data of distance, temperature and rad. vel but still we have a good data homogenity. Working on this data we found that:
the total average of rad. vel. is +36 km/sec;
the 40 nearest stars have an average rad. vel. of 31 km/sec, while the other ones have 41 km/sec;
the 20 nearest stars have an average rad.vel. of 19 km/sec, while the 20 farest have 55 km/sec;
the 40 warmest stars have an average rad. vel. of 49 km/sec, while the other ones have 22 km/sec;
the 20 warmest stars have an average rad.vel of 53 km/sec, while the 20 coldest have only 8 km/sec....
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