Dictionary of Nomenclature of Celestial Objects

NN> (Nos 1-100). Table 1: <BIG NN> N=? Table 1: <BIS NN> (Nos 1-61)?
Auth.:MICKAELIAN A.M.
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)?

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