Dictionary of Nomenclature of Celestial Objects
(Last update: 13-Jan-2022)

Result of query: info cati M97c]$

Details on Acronym:   [M97c]
   [M97c] (Mickaelian, 1997) Write:<<[M97c] NNNa>> N: 315+ Object:?  (SIMBAD class: Unknown = Object of unknown nature) Note:Optical identif. of IRAS sources on First Biurakan Survey plates. Objects are Stars, or QSO, Galaxies... See BIG for galaxies, BIS for stars. Ref:=1997Ap.....40....1M byMICKAELIAN A.M. Astrophysics, 40, 1-9 (1997) Optical identification of 100 IRAS point sources at high galactic latitude. oGalaxies 'BIG NN' and stars 'BIS NN' are not numbered here, they are respectively the galaxies and the stars included in [M97c] NNN objects. oTable 1: <[M97c] NNN> (Nos 1-100). Table 1: <BIG NN> N=? Table 1: <BIS NN> (Nos 1-61)? Ref:=1997Ap.....40..379M byMICKAELIAN A.M. , GIGOYAN K.S., RUSSEIL D. Astrophysics, 40, 379-389 (1997) Optical identification of IRAS point sources on the basis of low-dispersion FBS spectra. II. oGalaxies 'BIG NN' are not numbered here, they are added to the galaxies in the first '[M97c]' reference: 1997Ap.....40....1M. oTable 1: <[M97c] NNNa> (Nos 101-158) N=68. Table 1: <BIG NNN> N=? Ref:=1998Ap.....41..161M byMICKAELIAN A.M. , GIGOYAN K.S. Astrophysics, 41, 161-169 (1998) Optical identification of IRAS point sources on the basis of low-dispersion FBS spectra. III. oGalaxies 'BIG NNN' are not numbered here, they are added to the galaxies in the first '[M97c]' references. oTable 1: <[M97c] NNNa> (Nos 159-206) N=62. Table 1: <BIG NNN> N=? Ref:=1998Ap.....41..232M byMICKAELIAN A.M. , GIGOYAN K.S. Astrophysics, 41, 232-238 (1998) Optical identification of IRAS point sources on the basis of low-dispersion FBS spectra. IV. oGalaxies 'BIG NNN' are not numbered here, they are added to the galaxies in the first '[M97c]' references. oTable 1: <[M97c] NNNa> (Nos 207-240) N=51. Table 1: <BIG NNN> N=? Ref:=1999Ap.....42...37G byGIGOYAN K.S. , MICKAELIAN A.M. Astrophysics, 42, 37-42 (1999) Optical identification of IRAS point sources based on low-dispersion spectra from the First Byurakan Survey. V. oStars 'BIS NNN' are not numbered here, they are added to the stars in the first '[M97c]' reference: 1997Ap.....40....1M. oTable 1: <[M97c] NNN> N=19 among (Nos 242-315). Table 1: <BIS NNN> (Nos 62-137)? Originof the Acronym: S = Created by Simbad, the CDS Database

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