Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Mar-2024)

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: Variable* = 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)