| on. Astrophys., 640A, 92-92 (2020) | |
| Using classical Cepheids to study the far side of the Milky Way disk. I. Spectroscopic classification and the metallicity gradient. | |
| o | Tables 1+3: <[MSR2020] BNN> (Nos B01-B24). Tables 2+4: <[MSR2020] DNN> (Nos D01-D21). |
| Auth.: | MINNITI J.H.+ |
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