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 |
| by | MICKAELIAN A.M. |
| Astrophysics, 40, 1-9 (1997) | |
| Optical identification of 100 IRAS point sources at high galactic latitude. | |
| o | Galaxies 'BIG NN' and stars 'BIS NN' are not numbered here, they are respectively the galaxies and the stars included in [M97c] NNN objects. |
| o | Table 1: <[M97c] NNN> (Nos 1-100). Table 1: <BIG NN> N=? Table 1: <BIS NN> (Nos 1-61)? |
| Ref: | =1997Ap.....40..379M |
| by | MICKAELIAN 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. | |
| o | Galaxies 'BIG NN' are not numbered here, they are added to the galaxies in the first '[M97c]' reference: 1997Ap.....40....1M. |
| o | Table 1: <[M97c] NNNa> (Nos 101-158) N=68. Table 1: <BIG NNN> N=? |
| Ref: | =1998Ap.....41..161M |
| by | MICKAELIAN 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. | |
| 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=? |
| 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)? |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |