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Details on Acronym: [BKB99]
[BKB99] (Becker+Kawai+Brinkmann+, 1999) Write:<<[BKB99] PSR B1055-52 CN>>
<<[BKB99] PSR B1055-52 NN>>
<<[BKB99] PSR B0656+14 CN>>
<<[BKB99] PSR B0656+14 NN>>
<<[BKB99] Geminga CN>>
<<[BKB99] Geminga NN>> N: 3+13+2+15+8+23 Object:(X) (SIMBAD class: X = X-ray Source) Stat:is completely incorporated in Simbad Note:Analysis of archival ASCA, ROSAT and BeppoSAX data around PSR B1055-52, PSR B0656+14, and Geminga pulsar.
PSR B1055-52:
(Nos C1-C2, C4), X-ray sources observed from BeppoSAX. Map Fig.2. Sources C1 and C2 were interpreted as clumps in [SSG97], from ASCA observations. (Nos 1-13), X-ray sources observed from ROSAT PSPC. Map Fig.3.
PSR B0656+14:
(Nos C1-C3), X-ray sources observed from ASCA. Map Fig.5. (Nos 1-15), X-ray sources observed from ROSAT PSPC. Map Fig.6.
Geminga:
(Nos C1-C8), X-ray sources observed from ASCA. Map Fig.8. (Nos 1-23), X-ray sources observed from ROSAT PSPC. Map Fig.9. Ref:=1999A&A...352..532B byBECKER W. , KAWAI N., BRINKMANN W., MIGNANI R. Astron. Astrophys., 352, 532-542 (1999) The putative pulsar-wind nebulae of the three Musketeers PSR B1055-52, B0656+14 and Geminga revisited. oTable 1: <[BKB99] PSR B1055-52 CN> (Nos C1-C2, C4). Table 2: <[BKB99] PSR B1055-52 NN> (Nos 1-13). Table 3: <[BKB99] PSR B0656+14 CN> (Nos C1-C3), <[BKB99] PSR B0656+14 NN> (Nos 1-15). Table 4: <[BKB99] Geminga CN> (Nos C1-C8), <[BKB99] Geminga NN> (Nos 1-23). Originof the Acronym: S = Created by Simbad, the CDS Database
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