Strong pulses detected from rotating radio transient J1819 - 1458

Astronomy and Astrophysics

Volumn 530, Issue , 2011, Pages

  Hu, H D ^a,b   Esamdin, A ^a   Yuan, J P ^a   Liu, Z Y ^a   Xu, R X ^c   Li, J ^a,b   Tao, G C ^a,b   Wang, N ^a  

^a Chinese Academy of Sciences   (China)

^b UNIVERSITY OF CHINESE ACADEMY OF SCIENCES   (China)

^c PEKING UNIVERSITY   (China)

Author keywords

pulsars: individual: J1819 1458; stars: neutron

Indexed keywords

ARRIVAL TIME; CENTRAL FREQUENCY; CUMULATIVE PROBABILITY DISTRIBUTION; DISPERSION MEASURE; HIGH INTENSITY; POWER LAW; PULSARS: INDIVIDUALS; SINGLE PULSE; STARS: NEUTRON; STATISTICAL PROPERTIES;

STATISTICAL METHODS; TELESCOPES;

PROBABILITY DISTRIBUTIONS;

EID: 79955827266     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015953     Document Type: Article

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