Dictionary of Nomenclature of Celestial Objects
(Last update: 11-Oct-2019)

Result of query: info cati p$

Details on Acronym:   OP
   OP (Ohio univ., P stands for 14th hour of RA) ====>Equivalent to: Ohio Originof the Acronym: L = Found in the literature
Details on Acronym:   P
   P (Prata) (Not yet in Simbad) Write:<<P P>> Object:HVC  (SIMBAD class: HVCld = High-velocity Cloud) in source:NAME HVC CLOUD K Ref:=1968BAN....20...33H byHULSBOSCH A.N.M. Bull. Astron. Inst. Netherlands, 20, 33-39 (1968) High-velocity hydrogen complexes at high galactic latitudes. o<[H68] A>, <[H68] AC>, <[H68] AC R> (Nos I to III), <[H68] B>, <[H68] C>, <[H68] C R> (Nos I to III), <[H68] K>, <[H68] M>, <[H68] M R> (Nos I to II), <[H68] P>, <[H68] Sh>, <[H68] Sm>, <[H68] SP> Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   P
   P (Pike) (Not yet in Simbad) ***** Avoid the usage of P, prefer [PD64]
Details on Acronym:   P
   P (Peretto+Fuller) (Not yet in Simbad) ====>Equivalent to: [PF2009] Originof the Acronym: L (2010ApJ...723..915R)
Details on Acronym:   P
   P (PN) ***** Avoid the usage of P, prefer Ford Originof the Acronym: L (2006MNRAS.369...97H)
Details on Acronym:   P
   P (Mathewson) Note:HVC Complex P ***** Avoid the usage of P, prefer [H68] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   P
   P (Principal Galaxies Catalog) ***** Avoid the usage of P, prefer LEDA Originof the Acronym: L (2000A&AS..146..359K)
Details on Acronym:   P
   P (Parker) ***** Avoid the usage of P, prefer [P93] Originof the Acronym: L (1998AJ....116.1708R)
Details on Acronym:   P
   P (Parenago) ***** Avoid the usage of P, prefer Parenago
Details on Acronym:   P
   P (Pellet) ***** Avoid the usage of P, prefer [PAV78] Originof the Acronym: L = Found in the literature
Details on Acronym:   P
   P (Parker+) ***** Avoid the usage of P, prefer PGMW Originof the Acronym: L = Found in the literature
Details on Acronym:   P
   P (Partridge) ***** Avoid the usage of P, prefer [PHR86] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   P
   P (Parkes obs.) ***** Avoid the usage of P, prefer PKS Originof the Acronym: L = Found in the literature
Details on Acronym:   P
   P (Pluto occult.) ***** Avoid the usage of P, prefer Pluto Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   P
   P (Parsamian+) ***** Avoid the usage of P, prefer PP Originof the Acronym: L (1983ApJ...273..624C)
Details on Acronym:   P
   P (Pulsar) ***** Avoid the usage of P, prefer PSR Originof the Acronym: L = Found in the literature
Details on Acronym:   P
   P (Palomar survey) ***** Avoid the usage of P, prefer PSS Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   P
   P (Petite vitesse) ***** Avoid the usage of P, prefer PV Originof the Acronym: L = Found in the literature
Details on Acronym:   P
   P (Preibisch+) ***** Avoid the usage of P, prefer [PZH96] Originof the Acronym: L (1998ApJ...508..347L)
Details on Acronym:   P
   P (Prager) Write:<<SV* P NNNN>> Object:V*  (SIMBAD class: V* = Variable Star) Note:V* Nomenclature. Auth.:PRAGER
Details on Acronym:   Cl* Berkeley 17 P
   Cl* Berkeley 17 P (Phelps) Write:<<Cl* Berkeley 17 P 1-NNN>>
<<Cl* Berkeley 17 P 2-NNN>> N: 806+448 Object:*inCl Rem:Format '1-NNN' stars in the cluster field.

Format '2-NNN' stars in the off-cluster control field.
Ref:=1997ApJ...483..826P byPHELPS R.L. Astrophys. J., 483, 826-836 (1997) Berkeley 17: the oldest open cluster? ofig1a, 1b: <Cl* Berkeley 17 P 1-NNN> (Nos 1-1 to 1-806). fig2: <Cl* Berkeley 17 P 2-NNN> (Nos 2-1 to 2-448). =E=Catalogue in electronic form as J/ApJ/483/826
Details on Acronym:   Cl* Haffner 17 P
   Cl* Haffner 17 P (Pedreros) Write:<<Cl* Haffner 17 P NNN>> N: 123 Object:*inCl Ref:=2000RMxAA..36...13P byPEDREROS M.H. Rev. Mex. Astron. Astrofis., 36, 13-22 (2000) CCD photometry of the open clusters NGC 2671 and anonymous Haffner 17 (C0749-317). oTable 2: <Cl* NGC 2671 P NN> (Nos 1-62). Table 3: <Cl* Haffner 17 P NNN> (Nos 1-123, No. 62 missing).
Details on Acronym:   Cl* IC 4665 P
   Cl* IC 4665 P (Prosser) Write:<<Cl* IC 4665 P NNN>> N: 414 Object:*inCl Ref:=1993AJ....105.1441P byPROSSER C.F. Astron. J., 105, 1441-1454 (1993) The open cluster IC 4665. oTables 1-4: <Cl* IC 4665 P NNN> (Nos 1-414).
Details on Acronym:   Cl* IC 4665 P
   Cl* IC 4665 P (Prosser) Write:<<Cl* IC 4665 P VN>> N: 1 Object:*inCl Ref:=1995IBVS.4223....1P byPROSSER C.F. IAU Inform. Bull. Var. Stars, 4223, 1-2 (1995) New variable in Ophiuchus. o<Cl* IC 4665 P V1> N=1
Details on Acronym:   Cl* IC 4665 Pro
   Cl* IC 4665 Pro (Prosser) ====>Equivalent to: Cl* IC 4665 P
Details on Acronym:   Cl* NGC 104 P
   Cl* NGC 104 P (Paresce+) ====>Equivalent to: Cl* NGC 104 PSM Originof the Acronym: L = Found in the literature
Details on Acronym:   Cl* NGC 1466 P
   Cl* NGC 1466 P (Penny) Write:<<Cl* NGC 1466 P A>> N: 10 Object:*inCl Ref:=1981MNRAS.197..693P byPENNY A.J. Mon. Not. R. Astron. Soc., 197, 693-698 (1981) Three UBV sequences in the LMC. o<Cl* NGC 1466 P A> (Nos A-H, M, P), <Cl* NGC 2214 P A> (Nos A-D, F, G), <Cl* NGC 2257 P A> (Nos A, B, E-N, P, Q), <Cl* NGC 2257 P AA> (Nos AA, AB, KK>
Details on Acronym:   Cl* NGC 1502 P
   Cl* NGC 1502 P (Purgathofer) ====>Equivalent to: NGC 1502
Details on Acronym:   Cl* NGC 1907 P
   Cl* NGC 1907 P (Purgathofer) ====>Equivalent to: NGC 1907
Details on Acronym:   Cl* NGC 1977 P
   Cl* NGC 1977 P (Parenago) ====>Equivalent to: Parenago
Details on Acronym:   Cl* NGC 2175 P
   Cl* NGC 2175 P (Pismis) ====>Equivalent to: NGC 2175
Details on Acronym:   Cl* NGC 2214 P
   Cl* NGC 2214 P (Penny) Write:<<Cl* NGC 2214 P A>> N: 6 Object:*inCl Ref:=1981MNRAS.197..693P byPENNY A.J. Mon. Not. R. Astron. Soc., 197, 693-698 (1981) Three UBV sequences in the LMC. o<Cl* NGC 1466 P A> (Nos A-H, M, P), <Cl* NGC 2214 P A> (Nos A-D, F, G), <Cl* NGC 2257 P A> (Nos A, B, E-N, P, Q), <Cl* NGC 2257 P AA> (Nos AA, AB, KK>
Details on Acronym:   Cl* NGC 2257 P
   Cl* NGC 2257 P (Penny) Write:<<Cl* NGC 2257 P A>>
<<Cl* NGC 2257 P AA>> N: 16+3 Object:*inCl Ref:=1981MNRAS.197..693P byPENNY A.J. Mon. Not. R. Astron. Soc., 197, 693-698 (1981) Three UBV sequences in the LMC. o<Cl* NGC 1466 P A> (Nos A-H, M, P), <Cl* NGC 2214 P A> (Nos A-D, F, G), <Cl* NGC 2257 P A> (Nos A, B, E-N, P, Q), <Cl* NGC 2257 P AA> (Nos AA, AB, KK>
Details on Acronym:   Cl* NGC 2264 P
   Cl* NGC 2264 P (Pennsylvania univ.) ====>Equivalent to: NGC 2264
Details on Acronym:   Cl* NGC 2539 P
   Cl* NGC 2539 P (Pesch) ====>Equivalent to: NGC 2539
Details on Acronym:   Cl* NGC 2671 P
   Cl* NGC 2671 P (Pedreros) Write:<<Cl* NGC 2671 P NN>> N: 62 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2000RMxAA..36...13P byPEDREROS M.H. Rev. Mex. Astron. Astrofis., 36, 13-22 (2000) CCD photometry of the open clusters NGC 2671 and anonymous Haffner 17 (C0749-317). oTable 2: <Cl* NGC 2671 P NN> (Nos 1-62). Table 3: <Cl* Haffner 17 P NNN> (Nos 1-123, No. 62 missing).
Details on Acronym:   Cl* NGC 288 P
   Cl* NGC 288 P (Penny) ====>Equivalent to: NGC 288
Details on Acronym:   Cl* NGC 5053 P
   Cl* NGC 5053 P (Purtgathofer) Write:<<Cl* NGC 5053 P A>> N: 20 Object:*inCl Ref:=1966MiWie..13...15P byPURGATHOFER A. Mitt. Univ. Sternw. Wien, 13, 15-21 (1966) Der Kugelsternhaufen NGC 5053. o<Cl* NGC 5053 P A> (Nos A-U, I missing).
Details on Acronym:   Cl* NGC 6366 P
   Cl* NGC 6366 P (Pike) Write:<<Cl* NGC 6366 P NNN # 3 digits>> N: 68+70+54+72 Object:*inCl Rem:Table II:
in Quadrant I (Nos 101-174), (sometimes written I-NN),
in Quadrant II (Nos 201-356),(sometimes written II-NN),
in Quadrant III (Nos 301-356),(sometimes written III-NN),
in Quadrant IV (Nos 401-472) (sometimes written IV-NN) Ref:=1976MNRAS.177..257P byPIKE C.D. Mon. Not. R. Astron. Soc., 177, 257-264 (1976) The metal rich globular cluster NGC 6366. oTable II: <Cl* NGC 6366 P NNN> (Nos 101-174, 201-272, 301-356, 401-472)
Details on Acronym:   Cl* NGC 663 P
   Cl* NGC 663 P (Pietrzynski) Write:<<Cl* NGC 663 P VN>> N: 7 Object:*inCl Ref:=1996AcA....46..357P byPIETRZYNSKI G. Acta Astron., 46, 357-360 (1996) Variable stars in the young open cluster NGC 663. o<Cl* NGC 663 P VN> (Nos V1-V2) Ref:=1997AcA....47..211P byPIETRZYNSKI G. Acta Astron., 47, 211-223 (1997) A CCD search for variable stars in young open cluster NGC 663. o<Cl* NGC 663 P VN> (Nos V3-V7)
Details on Acronym:   Cl* NGC 6656 P
   Cl* NGC 6656 P (Philip) Write:<<Cl* NGC 6656 P NN>> N: 3 Object:*inCl Stat:is completely incorporated in Simbad Rem:from Philp, 1974, private communication Ref:=1976PASP...88..849H byHESSER J.E. Publ. Astron. Soc. Pac., 88, 849-859 (1976) The interstellar reddening in the direction of four low-latitude globular clusters. oT.V: PG = Cl* NGC 6656 PG NN, P A are from Philp, 1974, private communication. oTable I: <Cl* NGC 6304 H NN> (Nos 1-25). Table II: <Cl* NGC 6352 H NN> (Nos 1-22). Table IV: <Cl* NGC 6441 H NN> (Nos 1-14). Table V: <Cl* NGC 6656 P A> (Nos A, C), <Cl* NGC 6656 H NN> (Nos 40, 43, 46).
Details on Acronym:   Cl* NGC 6819 P
   Cl* NGC 6819 P (Purgathofer) Write:<<Cl* NGC 6819 P NN>> N: 38 Object:*inCl Ref:=1966MiWie..13....7P byPURGATHOFER A. Mitt. Univ. Sternw. Wien, 13, 7-None (1966) Der galaktische Sternhaufen NGC 6819. o<Cl* NGC 6819 P NN> (Nos 1-38).
Details on Acronym:   Cl* NGC 6883 P
   Cl* NGC 6883 P (Purgathofer) ====>Equivalent to: NGC 6883
Details on Acronym:   Cl* NGC 7790 P
   Cl* NGC 7790 P (Pedreros+) ====>Equivalent to: Cl* NGC 7790 PMF
Details on Acronym:   Cl* Trumpler 9 P
   Cl* Trumpler 9 P (Pismis) ====>Equivalent to: Cl Trumpler 9
Details on Acronym:   Cl* VDB 1 P
   Cl* VDB 1 P (Preston) Write:<<Cl* VDB 1 P N>> N: 6 Object:*inCl Ref:=1964PASP...76..165P byPRESTON G.W. Publ. Astron. Soc. Pac., 76, 165-168 (1964) Spectral types of stars in the field of CV Monocerotis. oTable I: Stars (C-U) are 'CL VDB 1 NN' (NOs 3-21) in SIMBAD oTable II: <Cl* VDB 1 P N> (Nos 1-6)

© Université de Strasbourg/CNRS

    • Contact