Dictionary of Nomenclature of Celestial Objects
(Last update: 24-Jan-2023)

Result of query: info cati Cl* NGC 5904 SAW$

Details on Acronym:   Cl* NGC 5904 HSH
   Cl* NGC 5904 HSH (H. Sawyer-Hogg) ====>Equivalent to: Cl* NGC 5904 Saw
Details on Acronym:   Cl* NGC 5904 Saw
   Cl* NGC 5904 Saw (Sawyer-Hogg) Write:<<Cl* NGC 5904 Saw VNNN>> N: 181 Object:*inCl Ref:=1973PDDO....3....6S bySAWYER HOGG H. Publ. David Dunlap Obs., 3, 6-75 (1973) A third catalogue of variable stars in globular clusters comprising 2119 entries. oref. is in Vol. 3, No. 6 o<Cl* NGC NNNN SAW VNNN>, <Cl* Palomar NN SAW VNNN>, <Cl* IC NNNN SAW VNNN>, <Cl* Haute-Provence 1 SAW VNN>, <NAME Tonantzintla 2>. Ref:=1987ATsir1502....7K byKADLA Z.I. , GERASHCHENKO A.N., JABLOKOVA N.V., IRKAEV B.N. Astron. Tsirk., 1502, 7-8 (1987) New variable stars in the globular cluster M 5. oV95 = KUST 374 not 378, V96 = KUST 527 not 526, V103 = KUST 667 not 583. o<Cl* NGC 5904 Saw VNNN> (Nos V104-V114) Ref:=1988ATsir1526....6K byKRAVTSOV V.V. Astron. Tsirk., 1526, 6-None (1988) New variable stars in the globular cluster M 5. o<Cl* NGC 5904 Saw VNNN> (Nos V115-V131) Ref:=1991PAZh...17.1101K byKRAVTSOV V.V. Pis'ma Astron. Zh., 17, 1101-1104 (1991) Two new variables in the central region of the globular cluster M 5. o<Cl* NGC 5904 Saw VNNN> (Nos V132-V133) Ref:=1996ApJ...470..910S bySANDQUIST E.L. , BOLTE M., STETSON P.B., HESSER J.E. Astrophys. J., 470, 910-952 (1996) CCD photometry of the globular cluster M5. I. The color-magnitude diagram and luminosity functions. oTable 2: <Cl* NGC 5904 SBS NNN> N=118 among (Nos 1-141). Table 8: <Cl* NGC 5904 Saw VNNN> (Nos V134-V141) Ref:=1999MNRAS.306..815C byCAPUTO F. , CASTELLANI V., MARCONI M., RIPEPI V. Mon. Not. R. Astron. Soc., 306, 815-827 (1999) RR Lyrae variables in M5 as a test of pulsational theory. oTable 1: <Cl* NGC 5904 Saw VNNN> (Nos V142-V159). Ref:=1999MNRAS.310..759O byOLECH A. , WOZNIAK P.R., ALARD C., KALUZNY J., THOMPSON I.B. Mon. Not. R. Astron. Soc., 310, 759-764 (1999) Variable stars in the globular cluster M5: application of the image subtraction method. o<Cl* NGC 5904 Saw VNNN> (Nos V160-V163). Ref:=2004ApJ...611..323S bySANDQUIST E.L. , BOLTE M. Astrophys. J., 611, 323-337 (2004) Exploring the upper red giant and asymptotic giant branches: the globular cluster M5. oTable 1: <Cl* NGC 5904 SB 1-NNN> (Nos 1-1 to 1-105). Table 2: <Cl* NGC 5904 SB 2-NNN> (Nos 2-1 to 2-438). Table 3: <Cl* NGC 5904 SAW VNNN> (No. V169) added. Table 4: <Cl* NGC 5904 SB 4-NNN> (Nos 4-1 to 4-446). Ref:=2015IBVS.6137....1A byARELLANO FERRO A. , BRAMICH D.M., GIRIDHAR S., LUNA A., MUNEER S. IAU Inform. Bull. Var. Stars, 6137, 1 (2015) New variables in M5 (NGC 5904) and some identification corrections. oTable 4: <Cl* NGC 5904 Saw VNNN> (Nos V170-V181). =E=Catalogue in electronic form as <V/97/>

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