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| Ton S 145 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST11:07:01 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
1962BOTT....3...37H |
233 | 109 | Faint blue stars in the region near the South Galactic Pole. | HARO G. and LUYTEN W.J. | |||||
|
2000AJ....119..241L |
190 | 29 | The Montreal-Cambridge-Tololo survey of southern subluminous blue stars: the south Galactic cap. | LAMONTAGNE R., DEMERS S., WESEMAEL F., et al. | |||||
|
2016MNRAS.459.4343K |
16 | D | 389 | 6 | The Edinburgh-Cape Blue Object Survey - V. The end: Partial Zones 4-6: Galactic latitudes -50deg > b > -90deg. | KILKENNY D., WORTERS H.L., O'DONOGHUE D., et al. | |||
|
2017A&A...600A..50G |
16 | D | 5613 | 59 | The population of hot subdwarf stars studied with Gaia. I. The catalog of known hot subdwarf stars. | GEIER S., OSTENSEN R.H., NEMETH P., et al. | |||
|
2019A&A...621A..38G |
16 | D | 1 | 39805 | 85 | The population of hot subdwarf stars studied with Gaia. II. The Gaia DR2 catalogue of hot subluminous stars. | GEIER S., RADDI R., GENTILE FUSILLO N.P., et al. | ||
|
2019MNRAS.482.4570G |
16 | D | 1 | 486646 | 296 | A Gaia Data Release 2 catalogue of white dwarfs and a comparison with SDSS. | GENTILE FUSILLO N.P., TREMBLAY P.-E., GANSICKE B.T., et al. | ||
|
2020A&A...635A.193G |
16 | D | 2 | 6177 | 44 | The population of hot subdwarf stars studied with Gaia. III. Catalogue of known hot subdwarf stars: Data Release 2. | GEIER S. | ||
|
2022A&A...662A..40C |
17 | D | 2 | 62976 | 9 | The population of hot subdwarf stars studied with Gaia. IV. Catalogues of hot subluminous stars based on Gaia EDR3. | CULPAN R., GEIER S., REINDL N., et al. | ||
| 2023MNRAS.518.6223I | 17 | D | 4 | 88 | 5 | Hyper-runaway and hypervelocity white dwarf candidates in Gaia Data Release 3: Possible remnants from Ia/Iax supernova explosions or dynamical encounters. | IGOSHEV A.P., PERETS H. and HALLAKOUN N. |