|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| [BGK2002] A10 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST04:07:53 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 2002ApJ...567..277B | 85 | 51 | Spectroscopy of blue supergiants in the spiral galaxy NGC 300. | BRESOLIN F., GIEREN W., KUDRITZKI R.-P., et al. | |||||
| 2004ApJ...600..182B | 31 | 26 | On the photometric variability of blue supergiants in NGC 300 and its impact on the flux-weighted gravity-luminosity relationship. | BRESOLIN F., PIETRZYNSKI G., GIEREN W., et al. | |||||
| 2005ApJ...634.1020B | 62 | 28 | The Araucaria project: the effect of blending on the Cepheid distance to NGC 300 from Advanced Camera for Surveys images. | BRESOLIN F., PIETRZYNSKI G., GIEREN W., et al. | |||||
| 2005AcA....55..195D | 3 | 8 | On the nature of regular pulsation in two LBV stars of NGC 300. | DZIEMBOWSKI W.A. and SLAWINSKA J. | |||||
| 2008ApJ...681..269K | 16 | D | 1 | 52 | 132 | Quantitative spectroscopy of 24 A supergiants in the Sculptor galaxy NGC 300: flux-weighted gravity-luminosity relationship, metallicity, and metallicity gradient. | KUDRITZKI R.-P., URBANEJA M.A., BRESOLIN F., et al. | ||
| 2009ApJ...700..309B | 38 | X | 1 | 76 | 224 | Extragalactic chemical abundances: do H II regions and young stars tell the same story? the case of the spiral galaxy NGC 300. | BRESOLIN F., GIEREN W., KUDRITZKI R.-P., et al. | ||
| 2013MNRAS.433.1246S | 554 | D | S X C | 13 | 25 | 69 | Evolution of blue supergiants and α Cygni variables: puzzling CNO surface abundances. | SAIO H., GEORGY C. and MEYNET G. | |
| 2014MNRAS.439L...6G | 156 | X F | 3 | 7 | 26 | The puzzle of the CNO abundances of α Cygni variables resolved by the Ledoux criterion. | GEORGY C., SAIO H. and MEYNET G. |