Variation of Emission-Line Strengths across M31
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| Veröffentlicht in: | Astrophys. J. 177: No. 1, 31-44(1 Oct 1972) 31-44(1 Oct 1972), 1972-01, Vol.177, p.31 |
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| container_title | Astrophys. J. 177: No. 1, 31-44(1 Oct 1972) |
| container_volume | 177 |
| creator | Rubin, Vera C. Krishna Kumar, C. Ford, W. Kent, Jr |
| description | |
| doi_str_mv | 10.1086/151684 |
| format | Article |
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| fulltext | fulltext |
| identifier | ISSN: 0004-637X |
| ispartof | Astrophys. J. 177: No. 1, 31-44(1 Oct 1972), 1972-01, Vol.177, p.31 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_crossref_primary_10_1086_151684 |
| source | Alma/SFX Local Collection |
| subjects | CHEMICAL COMPOSITION DISTANCE EMISSION SPECTRA GALAXIES GALAXIES/nitrogen abundance in M31, (E) GALAXIES/oxygen abundance in M31, (E) GALAXIES/spectra of M31, variation of emission-line strengths in, (E) H2 REGIONS HII REGIONS/spectra of, in M31, (E) N56500 -Physics (Astrophysics & Cosmology)-Galaxies NITROGEN NITROGEN/abundance in M31, (E) OXYGEN OXYGEN/abundance in M31, (E) VARIATIONS |
| title | Variation of Emission-Line Strengths across M31 |
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