Citation:Twin ejection of Blue straggler and red straggler at the "dynamical stability limit turning towards unbalancing at the point of unbalancing a diagonolization squeezing between short and longer waves for a double ejection A new type of Quantum dynamical ejection at the meeting point of binary pars dealing with pi dynamical unstability may be for a very important discovery paved the way for seeding rahu and kethu pi dinmaics a very important discovery as well as in pi dynamics of microchips Birth of a blue straggler star. Left: A normal star in a binary system gravitationally pulls in matter from an aging companion star that has swelled to a bloated red giant that is a few hundred times its original size. Right: After a couple hundred million years, the red giant star has burned out and collapsed to the white dwarf that shines intensely in ultraviolet wavelengths. The companion star has bulked up on hydrogen siphoned from the red giant to become much hotter, brighter and bluer. White dwarfs form when certain stars lose their outer atmospheres. The mass "must be going somewhere," Sankaravelayudhan says, "and that's to the companion normal star, which is close enough to attract the mass through gravity. Therefore, the white dwarf is left over after adding mass to a star, which becomes the blue straggler."Third force acting in between rotating binary stars at 180 pi phases calls for a region that you just can't cross -- if you go in there, you get ejected from the system, left side or right side called the "dynamical stability limit" as clockwise rotational or anticlockwise rotational sometimes as 180 degree phase Twin ejection also says Sankaravelayudhan Nandakumar Third force acting in between rotating binary stars calls for ejection of Rahu and Kethu out of solar and lunar ray interaction dynamics which is one of the greatest discovery of Quantum mechanics Birth of a blue straggler star. Left: A normal star in a binary system gravitationally pulls in matter from an aging companion star that has swelled to a bloated red giant that is a few hundred times its original size. Right: After a couple hundred million years, the red giant star has burned out and collapsed to the white dwarf that shines intensely in ultraviolet wavelengths. The companion star has bulked up on hydrogen siphoned from the red giant to become much hotter, brighter and bluer. White dwarfs form when certain stars lose their outer atmospheres. The mass "must be going somewhere," Sankaravelayudhan Nandakumar says, at the meeting balancing point of ejection becomes a dynamical unbalancing an attractive force becominga a net repulsive force of pi dynamics making it rotational clockwise or anticlockwise dynamics as the case may be. “and that's to the companion normal star, which is close enough to attract the mass through gravity. Therefore, the white dwarf is left over after adding mass to a star, which becomes the blue straggler." Hawking's Blue straggler ejected from Sagittarius archer-reg - 00227563
Journal Reference: 1. David P. Fleming, Rory Barnes, David E. Graham, Rodrigo Luger, Thomas R. Quinn. On The Lack of Circumbinary Planets Orbiting Isolated Binary Stars. Astrophysical Journal, 2018 [link] 2. Circumbinary castaways: Short-period binary systems can eject orbiting worlds 3. Natalie M. Gosnell, Robert D. Mathieu, Aaron M. Geller, Alison Sills, Nathan Leigh, Christian Knigge. IMPLICATIONS FOR THE FORMATION OF BLUE STRAGGLER STARS FROMHSTULTRAVIOLET OBSERVATIONS OF NGC 188. The Astrophysical Journal, 2015; 814 (2): 163 DOI: 10.1088/0004-637X/814/2/163