Dictionary of Nomenclature of Celestial Objects
(Last update: 26-Nov-2020)

Result of query: info cati WV$

Details on Acronym:   HVC
   HVC (High-Velocity Cloud) ***** Avoid the usage of HVC, prefer WV Originof the Acronym: L (1998AJ....116.1205S)
Details on Acronym:   WV
   WV (Wakker+Van Woerden)= (HVC) = (WvW) = (WvW91) = (WW) Write:<<WV NNN>> N: 561+? Object:HVC  (SIMBAD class: HVCld = High-velocity Cloud) Stat:is completely incorporated in Simbad Note:The numbering is ordered by dicreasing latitude. Ref:=1991A&A...250..509W byWAKKER B.P. , VAN WOERDEN H. Astron. Astrophys., 250, 509-532 (1991) Distribution and origin of high-velocity clouds. III. Clouds, complexes and populations. oTable 1: <WV NNN> (Nos 1-561). Table 3: <[H68] A> (Nos D, G, H, L), <[H68] AA> (Nos WA-WD), <NAME GCN Complex>, <NAME GCP Complex>, <NAME ACHV Complex>, <NAME ACVHV Complex>. Ref:=2002MNRAS.337..720C byCRAWFORD I.A. , LALLEMENT R., PRICE R.J., SFEIR D.M., WAKKER B.P., WELSH B.Y. Mon. Not. R. Astron. Soc., 337, 720-730 (2002) High-resolution observations of interstellar NaI and CaII towards the southern opening of the `Local Interstellar Chimney': probing the disc-halo connection. oFig.4: <WV NNN> N=5 among (Nos 607-627) added. Originof the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym:   WvW
   WvW (Wakker+van Woerden) ***** Avoid the usage of WvW, prefer WV Originof the Acronym: L (2002AJ....123..873P)
Details on Acronym:   WvW91
   WvW91 (Wakker+van Woerden, 1991) ***** Avoid the usage of WvW91, prefer WV Originof the Acronym: L (1999ApJ...523..163A)
Details on Acronym:   WW
   WW (Wakker+Van Woerden) ***** Avoid the usage of WW, prefer WV Originof the Acronym: L (2001ApJS..136..463W)
Details on Acronym:   Cl* NGC 188 KH
   Cl* NGC 188 KH (Kafka+Honeycutt) ====>Equivalent to: Cl* NGC 188 WV
Details on Acronym:   Cl* NGC 188 WV
   Cl* NGC 188 WV (WIYN Variable) Write:<<Cl* NGC 188 WV NN>> N: 51 Object:*inCl Ref:=2003AJ....126..276K byKAFKA S. , HONEYCUTT R.K. Astron. J., 126, 276-285 (2003) WIYN open cluster study. XV. Photometric monitoring of open clusters: new variables in NGC 188. oTables 2, 4: <Cl* NGC 188 WV NN> (Nos 1-51). Originof the Acronym: A = Assigned by the author(s)

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