Details on Acronym: BP
BP (Bailey+Pooley) Write:<<BP NNN>> N: 198 Object:(Rad) (SIMBAD class: Radio = Radio Source) Stat:is completely incorporated in Simbad Ref:=1968MNRAS.138...51B byBAILEY J.A. , POOLEY G.G. Mon. Not. R. Astron. Soc., 138, 51-66 (1968) Fan-beam observations of radio sources at 408 and 1407 MHz. oTable I: <BP NNN> (Nos 1-198) Originof the Acronym: L = Found in the literature
Details on Acronym: Cl* NGC 6871 BP
Cl* NGC 6871 BP (Bernabei+Polcaro) Write:<<Cl* NGC 6871 BP NN>> N: 10 Object:*inCl Ref:=2001A&A...366..817B byBERNABEI S. , POLCARO V.F. Astron. Astrophys., 366, 817-826 (2001) A search for peculiar objects in young open clusters. I. New emission line and late spectral type stars in NGC 6871. oTables 2, 3: <Cl* NGC 6871 BP N> (Nos 1-9). Ref:=2001A&A...371..123B byBERNABEI S. , POLCARO V.F. Astron. Astrophys., 371, 123-132 (2001) A search for peculiar objects in young open clusters. II. A new Be star, the optical counterpart of IRAS 19564+3224 and a new open cluster in Vulpecula. oin ref list FABREGAT J., REGLERO V., 1990MNRAS.247..407F instead of 249.414 o<NAME LOIANO 1>. p.126: <Cl* NGC 6871 BP NN> (No. 10) added. Table 3: <[BP2001] NN> (Nos 1-75).
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