scholarly journals A Quantitative Nonradial Oscillation Model for the Subpulses in PSR B0943+10

2008 ◽  
Vol 680 (1) ◽  
pp. 671-685 ◽  
Author(s):  
R. Rosen ◽  
J. Christopher Clemens
1988 ◽  
Vol 108 ◽  
pp. 99-100
Author(s):  
Masa-aki Kondo

Concerning the scattering of OB stars in the HR diagram (Humphry 1980), the effects of overshooting of convective core (Maeder 1984), mass loss (cf. chiosi and Maeder 1986), and generous stability criterion of semi-convection (Stothers and Chin 1976) have been discussed. Here, we will note the dredge up effect is caused by the sound waves emitted from a convective core.The sound mode of nonradial oscillation, with the spherical harmonics Ylm(θ, ϕ) and the frequency ω, can exist in the propagation zone, where the bottom boundary locates at the position of , and the upper boundary does near the photosphere. Here, Ll is called as the Lamb frequency, and cs is the sound velocity.


2018 ◽  
Vol 171 ◽  
pp. 155-164 ◽  
Author(s):  
Volodymyr Bulgakov ◽  
Simone Pascuzzi ◽  
Semjons Ivanovs ◽  
Grygorii Kaletnik ◽  
Vitaliy Yanovich

Author(s):  
Yong Li ◽  
Dechang Yang ◽  
Fang Liu ◽  
Yijia Cao ◽  
Christian Rehtanz

2019 ◽  
Vol 28 (09) ◽  
pp. 1950111 ◽  
Author(s):  
Grigoris Panotopoulos ◽  
Ilídio Lopes

We compute the lowest frequency nonradial oscillation modes of dilute axion stars. The effective potential that enters into the Schrödinger-like equation, several associated eigenfunctions and the large as well as the small frequency separations are shown as well.


2015 ◽  
Vol 6 (1) ◽  
Author(s):  
Hui Wang ◽  
Jian-Tao Wang ◽  
Ze-Xian Cao ◽  
Wen-Jun Zhang ◽  
Chun-Sing Lee ◽  
...  

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