Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Oct-2021)

Result of query: info cati TMC$
 REEMAN K.C.
     byGIBSON B.K.
, HENNING P.A., KILBORN V., KORIBALSKI B., KRAAN-KORTEWEG R.C., MALIN D.F., MINCHIN R.F., MOULD J.R., OOSTERLOO T., PRICE R.M., PUTMAN M.E., RYDER S.D., SADLER E.M., STAVELEY-SMITH L., STEWART I., STOOTMAN F., VAILE R.A., WEBSTER R.L., WRIGHT A.E.
 Astrophys. J., 524, 612-622 (1999)

    New galaxies discovered in the first blind H I survey of the Centaurus
    A group.
oTable 1: <[K99b] HIPASS JHHMM+DD> N=5, 3 are new.

Details on Acronym:   
   Y N=41 delta Scuti candidate stars and N=15 variable stars from the Taiwan-American Occultation Survey (TAOS).
More information at: http://taos.asiaa.sinica.edu.tw/index.php
See also [KPA2010]. Ref:=2010AJ....139..757K byKIM D.-W. , PROTOPAPAS P., ALCOCK C., BYUN Y.-I., KYEONG J., LEE B.-C., WRIGHT N.J., AXELROD T., BIANCO F.B., CHEN W.-P., COEHLO N.K., COOK K.H., DAVE R., KING S.-K., LEE T., LEHNER M.J., LIN H.-C., MARSHALL S.L., PORRATA R., RICE J.A., SCHWAMB M.E., WANG J.-H., WANG S.-Y., WEN C.-Y., ZHANG Z.-W. Astron. J., 139, 757-764 (2010) The Taiwan-American Occultation Survey project stellar variability. I. Detection of low-amplitude δ Scuti stars. oTable 3: <[KPA2010] NN> (Nos 1-41) = <TAOS FFF.NNNNN> N=41. Ref:=2010AJ....139.2026M byMONDAL S. , LIN C.C., CHEN W.P., ZHANG Z.-W., ALCOCK C., AXELROD T., BIANCO F.B., BYUN Y.-I., COEHLO N.K., COOK K.H., DAVE R. Ref:=1993AJ....105.1831T byTURBIDE L. , MOFFAT A.F.J. Astron. J., 105, 1831-1854 (1993) Precision photometry of young stellar groups towards the outer galactic disk and the galactic rotation curve. o<[TM93] SH 2-283 NNN> N=130. <[TM93] SH 2-284 NNN> N=235. <[TM93] SH 2-285 NNN> N=174. <[TM93] SH 2-289 NNN> N=358. <[TM93] SH 2-305 NN> N=95. <[TM93] SH 2-309 NNN> N=104. <CL* Bochum 2 TM NNN> N=136. <CL* Ruprecht 32 TM NNN> N=221
Details on Acronym:   [TM97]
   [TM97] (Thornley+Mundy, 1997)= (GMA) Write:<<[TM97] NGC 5055 NN>>
<<[TM97] NGC 4414 NN>> N: 17+13 Object:Giant Molecular Assoc.  (SIMBAD class: PartofG = Part of a Galaxy) Stat:is completely incorporated in Simbad in source:NGC 5055 in source:NGC 4414 Ref:=1997ApJ...484..202T byTHORNLEY M.D. , MUNDY L.G. Astrophys. J., 484, 202-221 (1997) Are flocculent spirals devoid of density waves? gas morphology and kinematics in NGC 5055. oTable 3: <[TM97] NGC 5055 NN> (Nos 1-17) Ref:=1997ApJ...490..682T byTHORNLEY M.D. , MUNDY L.G. Astrophys. J., 490, 682-697 (1997) Dynamic and stochastic influences on spiral structure in the flocculent spiral NGC 4414. oTable 2: <[TM97] NGC 4414 NN> (Nos 1-13) Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [TM98]
   [TM98] (Trentham+Mobasher, 1998) Write:<<[TM98] AN>> N: 18 Object:?  (SIMBAD class: Unknown = Object of unknown nature) Stat:is completely incorporated in Simbad in source:Coma Cluster = ACO 1656 Ref:=1998MNRAS.293...53T byTRENTHAM N. , MOBASHER B. Mon. Not. R. Astron. Soc., 293, 53-59 (1998) The discovery of a giant debris

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