Geodesic
Spherical quasi-Newtonian stellar pulsations in RTG
Teoretičeskaâ i matematičeskaâ fizika, Tome 106 (1996) no. 2, pp. 320-324

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It is shown that in Relativistic Theory of Gravity, in contrast to GTR the spherically symmetric stellar pulsations lead to the nonstatic behaviour of an external gravitational field. 
@article{TMF_1996_106_2_a12,
     author = {A. A. Vlasov},
     title = {Spherical {quasi-Newtonian} stellar pulsations in {RTG}},
     journal = {Teoreti\v{c}eska\^a i matemati\v{c}eska\^a fizika},
     pages = {320--324},
     publisher = {mathdoc},
     volume = {106},
     number = {2},
     year = {1996},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/TMF_1996_106_2_a12/}
}
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A. A. Vlasov. Spherical quasi-Newtonian stellar pulsations in RTG. Teoretičeskaâ i matematičeskaâ fizika, Tome 106 (1996) no. 2, pp. 320-324. http://geodesic.mathdoc.fr/item/TMF_1996_106_2_a12/