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Dictionary of Nomenclature of Celestial Objects
(Last update: 07-Feb-2010) |
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Details on Acronym: OPM
OPM (Ohio univ., P stands for 14th hour of RA, M stands for Medium-Velocity) ***** Avoid the usage of OPM, prefer Ohio Originof the Acronym: L = Found in the literature
Details on Acronym: PM
PM = (PMI) = (PMII) = (PMIII) (Proper Motion) Write:<<PM HHMMm+DDMMA>> Object:PM* (SIMBAD class: PM* = High proper-motion Star) Note:First ref. with PM*. See also LSR. Ref:=1979ApJS...39...89E byEGGEN O.J. Astrophys. J., Suppl. Ser., 39, 89-101 (1979) Catalogs of proper-motion stars. I. Stars brighter than visual magnitude 15 and with annual proper motion of 1" or more. oTable 1A: <PM HHMMm+DDMMA> N=430 Ref:=1980ApJS...43..457E byEGGEN O.J. Astrophys. J., Suppl. Ser., 43, 457-468 (1980) Catalogs of proper motion stars. II. Stars brighter than visual magnitude 15 and south of declination +30 with annual proper motion between 0"7 and 1"0. oCorrection in EGGEN O.J., 1983, Ap.J.Suppl. 51, 183-202 oTable 1: <PM HHMMm+DDMMA> N=434
Details on Acronym: PM
PM (Preite-Martinez) Write:<<PN PM 1-NNN>> or <<PN PM 2-NN>> N=340+48 Object:Poss. PN (SIMBAD class: PN? = Possible Planetary Nebula) Note:Table IV: PM 1-, list 1, N=340, sources with a high probability of being a PN
Table V: PM 2-, list 2, N=48, sources with a high probability of being non-PN, or only PN-related objects. Ref:=1988A&AS...76..317P byPREITE-MARTINEZ A. Astron. Astrophys., Suppl. Ser., 76, 317-330 (1988) Possible new planetary nebulae in the IRAS point source catalogue. oTable IV: <PN PM 1-NNN> N=340 , Table V: <PN PM 2-NN> N=48. Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: PM
PM (Parker+Morgan+) ***** Avoid the usage of PM, prefer PMR Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: PMI
PMI (Proper motion, I: (roman num.) 1st catalog) ***** Avoid the usage of PMI, prefer PM
Details on Acronym: PMII
PMII (Proper motion, II: (roman num.) 2nd catalog) ***** Avoid the usage of PMII, prefer PM
Details on Acronym: PMIII
PMIII (Proper motion, III: (roman num.) 3rd catalog) ***** Avoid the usage of PMIII, prefer PM
Details on Acronym: Cl* NGC 2439 PM
Cl* NGC 2439 PM (Paunzen+Maitzen) Write:<<Cl* NGC 2439 PM NNN>> N=113 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2002A&A...385..867P byPAUNZEN E. , MAITZEN H.M. Astron. Astrophys., 385, 867-873 (2002) CCD photometric search for peculiar stars in open clusters. III. NGC 2439, NGC 3960, NGC 6134, NGC 6192 and NGC 6451. oTable 4: <Cl* NGC 2439 PM NNN> (Nos 1-113). Table 5: <Cl* NGC 3960 PM NN> (Nos 1-93). Table 6: <Cl* NGC 6134 PM NNN> (Nos 1-102). Table 7: <Cl* NGC 6192 PM NN> (Nos 1-98). Table 8: <Cl* NGC 6451 PM NNN> (Nos 1-146). =E=Catalogue in electronic form as <J/A+A/385/867/>
Details on Acronym: Cl* NGC 2489 PM
Cl* NGC 2489 PM (Paunzen+Maitzen) Write:<<Cl* NGC 2489 PM NN>> N=59 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2001A&A...373..153P byPAUNZEN E. , MAITZEN H.M. Astron. Astrophys., 373, 153-158 (2001) CCD photometric search for peculiar stars in open clusters. II. NGC 2489, NGC 2567, NGC 2658, NGC 5281 and NGC 6208. oTable 4: <Cl* NGC 2489 PM NN> (Nos 1-59). Table 5: <Cl* NGC 2567 PM NN> (Nos 1-50). Table 6: <Cl* NGC 2658 PM NN> (Nos 1-55). Table7: <Cl* NGC 5281 PM NN> (Nos 1-30). Table 8: <Cl* NGC 6208 PM NN> (Nos 1-41).
Details on Acronym: Cl* NGC 2567 PM
Cl* NGC 2567 PM (Paunzen+Maitzen) Write:<<Cl* NGC 2567 PM NN>> N=50 Stat:is completely incorporated in Simbad Object:*inCl Ref:=2001A&A...373..153P byPAUNZEN E. , MAITZEN H.M. Astron. Astrophys., 373, 153-158 (2001) CCD photometric search for peculiar stars in open clusters. II. NGC 2489, NGC 2567, NGC 2658, NGC 5281 and NGC 6208. oTable 4: <Cl* NGC 2489 PM NN> (Nos 1-59). Table 5: <Cl* NGC 2567 PM NN> (Nos 1-50). Table 6: <Cl* NGC 2658 PM NN> (Nos 1-55). Table7: <Cl* NGC 5281 PM NN> (Nos 1-30). Table 8: <Cl* NGC 6208 PM NN> (Nos 1-41).
Details on Acronym: Cl* NGC 2658 PM
Cl* NGC 2658 PM (Paunzen+Maitzen) Write:<<Cl* NGC 2658 PM NN>> N=55 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2001A&A...373..153P byPAUNZEN E. , MAITZEN H.M. Astron. Astrophys., 373, 153-158 (2001) CCD photometric search for peculiar stars in open clusters. II. NGC 2489, NGC 2567, NGC 2658, NGC 5281 and NGC 6208. oTable 4: <Cl* NGC 2489 PM NN> (Nos 1-59). Table 5: <Cl* NGC 2567 PM NN> (Nos 1-50). Table 6: <Cl* NGC 2658 PM NN> (Nos 1-55). Table7: <Cl* NGC 5281 PM NN> (Nos 1-30). Table 8: <Cl* NGC 6208 PM NN> (Nos 1-41).
Details on Acronym: Cl* NGC 3960 PM
Cl* NGC 3960 PM (Paunzen+Maitzen) Write:<<Cl* NGC 3960 PM NN>> N=93 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2002A&A...385..867P byPAUNZEN E. , MAITZEN H.M. Astron. Astrophys., 385, 867-873 (2002) CCD photometric search for peculiar stars in open clusters. III. NGC 2439, NGC 3960, NGC 6134, NGC 6192 and NGC 6451. oTable 4: <Cl* NGC 2439 PM NNN> (Nos 1-113). Table 5: <Cl* NGC 3960 PM NN> (Nos 1-93). Table 6: <Cl* NGC 6134 PM NNN> (Nos 1-102). Table 7: <Cl* NGC 6192 PM NN> (Nos 1-98). Table 8: <Cl* NGC 6451 PM NNN> (Nos 1-146). =E=Catalogue in electronic form as <J/A+A/385/867/>
Details on Acronym: Cl* NGC 5281 PM
Cl* NGC 5281 PM (Paunzen+Maitzen) Write:<<Cl* NGC 5281 PM NN>> N=30 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2001A&A...373..153P byPAUNZEN E. , MAITZEN H.M. Astron. Astrophys., 373, 153-158 (2001) CCD photometric search for peculiar stars in open clusters. II. NGC 2489, NGC 2567, NGC 2658, NGC 5281 and NGC 6208. oTable 4: <Cl* NGC 2489 PM NN> (Nos 1-59). Table 5: <Cl* NGC 2567 PM NN> (Nos 1-50). Table 6: <Cl* NGC 2658 PM NN> (Nos 1-55). Table7: <Cl* NGC 5281 PM NN> (Nos 1-30). Table 8: <Cl* NGC 6208 PM NN> (Nos 1-41).
Details on Acronym: Cl* NGC 6134 PM
Cl* NGC 6134 PM (Paunzen+Maitzen) Write:<<Cl* NGC 6134 PM NNN>> N=102 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2002A&A...385..867P byPAUNZEN E. , MAITZEN H.M. Astron. Astrophys., 385, 867-873 (2002) CCD photometric search for peculiar stars in open clusters. III. NGC 2439, NGC 3960, NGC 6134, NGC 6192 and NGC 6451. oTable 4: <Cl* NGC 2439 PM NNN> (Nos 1-113). Table 5: <Cl* NGC 3960 PM NN> (Nos 1-93). Table 6: <Cl* NGC 6134 PM NNN> (Nos 1-102). Table 7: <Cl* NGC 6192 PM NN> (Nos 1-98). Table 8: <Cl* NGC 6451 PM NNN> (Nos 1-146). =E=Catalogue in electronic form as <J/A+A/385/867/>
Details on Acronym: Cl* NGC 6192 PM
Cl* NGC 6192 PM (Paunzen+Maitzen) Write:<<Cl* NGC 6192 PM NN>> N=98 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2002A&A...385..867P byPAUNZEN E. , MAITZEN H.M. Astron. Astrophys., 385, 867-873 (2002) CCD photometric search for peculiar stars in open clusters. III. NGC 2439, NGC 3960, NGC 6134, NGC 6192 and NGC 6451. oTable 4: <Cl* NGC 2439 PM NNN> (Nos 1-113). Table 5: <Cl* NGC 3960 PM NN> (Nos 1-93). Table 6: <Cl* NGC 6134 PM NNN> (Nos 1-102). Table 7: <Cl* NGC 6192 PM NN> (Nos 1-98). Table 8: <Cl* NGC 6451 PM NNN> (Nos 1-146). =E=Catalogue in electronic form as <J/A+A/385/867/>
Details on Acronym: Cl* NGC 6208 PM
Cl* NGC 6208 PM (Paunzen+Maitzen) Write:<<Cl* NGC 6208 PM NN>> N=41 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2001A&A...373..153P byPAUNZEN E. , MAITZEN H.M. Astron. Astrophys., 373, 153-158 (2001) CCD photometric search for peculiar stars in open clusters. II. NGC 2489, NGC 2567, NGC 2658, NGC 5281 and NGC 6208. oTable 4: <Cl* NGC 2489 PM NN> (Nos 1-59). Table 5: <Cl* NGC 2567 PM NN> (Nos 1-50). Table 6: <Cl* NGC 2658 PM NN> (Nos 1-55). Table7: <Cl* NGC 5281 PM NN> (Nos 1-30). Table 8: <Cl* NGC 6208 PM NN> (Nos 1-41).
Details on Acronym: Cl* NGC 6451 PM
Cl* NGC 6451 PM (Paunzen+Maitzen) Write:<<Cl* NGC 6451 PM NNN>> N=146 Object:*inCl Stat:is completely incorporated in Simbad Ref:=2002A&A...385..867P byPAUNZEN E. , MAITZEN H.M. Astron. Astrophys., 385, 867-873 (2002) CCD photometric search for peculiar stars in open clusters. III. NGC 2439, NGC 3960, NGC 6134, NGC 6192 and NGC 6451. oTable 4: <Cl* NGC 2439 PM NNN> (Nos 1-113). Table 5: <Cl* NGC 3960 PM NN> (Nos 1-93). Table 6: <Cl* NGC 6134 PM NNN> (Nos 1-102). Table 7: <Cl* NGC 6192 PM NN> (Nos 1-98). Table 8: <Cl* NGC 6451 PM NNN> (Nos 1-146). =E=Catalogue in electronic form as <J/A+A/385/867/>