ources on the basis of low-dispersion FBS spectra. III. | |
o | Galaxies 'BIG NNN' are not numbered here, they are added to the galaxies in the first '[M97c]' references. |
o | Table 1: <[M97c] NNNa> (Nos 159-206) N=62. Table 1: <BIG NNN> N=? |
Auth.: | MICKAELIAN A.M.+ |
Ref: | =1998Ap.....41..232M |
by | MICKAELIAN 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. | |
o | Galaxies 'BIG NNN' are not numbered here, they are added to the galaxies in the first '[M97c]' references. |
o | Table 1: <[M97c] NNNa> (Nos 207-240) N=51. Table 1: <BIG NNN> N=? |
Ref: | =1999Ap.....42...37G |
by | GIGOYAN 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. | |
o | Stars 'BIS NNN' are not numbered here, they are added to the stars in the first '[M97c]' reference: 1997Ap.....40....1M. |
o | Table 1: <[M97c] NNN> N=19 among (Nos 242-315). Table 1: <BIS NNN> (Nos 62-137)? |
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