Electronic Resource
Springer
Astrophysics and space science
12 (1971), S. 415-423
ISSN:
1572-946X
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract The effect of the source motion on the period variation of pulsars is investigated. For some pulsars, a velocity 100–300 km/s can give a Doppler contribution to the second period derivative P which is comparable or larger than the intrinsic variation predicted by theoretical models, whereas larger velocities are required in order to give an appreciable kinematic effect on the first derivative P. The possibility of experimental detection of P and proper motion for known pulsars is discussed.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00651430
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