Broadband pulsations from psr b1821-24: Implications for emission models and the pulsar population of M28

Astrophysical Journal

Volumn 778, Issue 2, 2013, Pages

  Johnson, T J ^a,f   Guillemot, L ^b   Kerr, M ^c   Cognard, I ^d,e   Ray, P S ^f   Wolff, M T ^f   Begin S ^g   Janssen, G H ^h   Romani, R W ^c   Venter, C ⁱ   Grove, J E ^f   Freire, P C C ^b   Wood, M ^c   Cheung, C C ^f   Casandjian, J M ^j   Stairs, I H ^k   Camilo, F ^l,m   Espinoza, C M ^h,n   Ferrara, E C ^o   Harding, A K ^o   Johnston, S ^p   Kramer, M ^b,h   Lyne, A G ^h   Michelson, P F ^c   Ransom, S M ^q   Shannon, R ^p   Smith, D A ^r   Stappers, B W ^h   Theureau, G ^d   Thorsett, S E ^s   more..

^a NATIONAL RESEARCH COUNCIL   (United States)

^b MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^c STANFORD UNIVERSITY   (United States)

^d LPCE CNRS   (France)

^e CNRS   (France)

^f NAVAL RESEARCH LABORATORY   (United States)

^g UNIVERSITÉ LAVAL   (Canada)

^h UNIVERSITY OF MANCHESTER   (United Kingdom)

ⁱ NORTH WEST UNIVERSITY   (South Africa)

^j CEA SACLAY   (France)

^k UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^l Columbia University ^*  (United States)

^m Arecibo Observatory   (Puerto Rico)

ⁿ PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^o NASA GODDARD SPACE FLIGHT CENTER   (United States)

^p CSIRO   (Australia)

^q NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^r CENTRE D ETUDES NUCLÉAIRES DE BORDEAUX GRADIGNAN   (France)

^s WILLAMETTE UNIVERSITY   (United States)

more..

Author keywords

24); gamma rays: stars; globular clusters: individual (M28); pulsars: individual (B1821

Indexed keywords

EID: 84887887226     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/778/2/106     Document Type: Article

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