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| V* HT Sgr , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST15:16:21 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1961AJ.....66..188H | 16 | 6 | 45 variable stars in VSF 193. | HOFFLEIT D. | |||||
| 1967IBVS..228....1H | 105 | 2 | Spectral types of long-period variables in Sagittarius. | HOUK N. | |||||
| 2000AAS...197.4804P | 9 | 0 | Nine lost variable stars recovered on nantucket plates. | PETERSON C.M., SAMUS N.N., HOLMES S., et al. | |||||
| 2001JAVSO..29..112S | 9 | 1 | Lost variables in Sagittarius and Cygnus recovered on Nantucket plates. | SAMUS N., PETERSON C., HOLMES S., et al. | |||||
|
2002AcA....52..397P |
14 | D | 2893 | 1175 | The All Sky Automated Survey. Catalog of variable stars. I. 0h -6h quarter of the Southern hemisphere. | POJMANSKI G. | |||
|
2016MNRAS.455.2216C |
16 | D | 1 | 650 | 41 | The age and structure of the Galactic bulge from Mira variables. | CATCHPOLE R.M., WHITELOCK P.A., FEAST M.W., et al. | ||
|
2016ApJS..227....6V |
16 | D | 1 | 2892 | 2 | Determination of pulsation periods and other parameters of 2875 stars classified as Mira in the All Sky Automated Survey (ASAS). | VOGT N., CONTRERAS-QUIJADA A., FUENTES-MORALES I., et al. | ||
|
2022ApJS..260...46I |
17 | D | 1 | 65989 | 11 | The OGLE Collection of Variable Stars: Nearly 66,000 Mira Stars in the Milky Way. | IWANEK P., SOSZYNSKI I., KOZLOWSKI S., et al. | ||
|
2023ApJS..264...20I |
17 | D | 1 | 65989 | 1 | A Three-dimensional Map of the Milky Way Using 66,000 Mira Variable Stars. | IWANEK P., POLESKI R., KOZLOWSKI S., et al. | ||
|
2023A&A...674A..15L |
17 | D | 1 | 1720610 | 15 | Gaia Data Release 3 The second Gaia catalogue of long-period variable candidates. | LEBZELTER T., MOWLAVI N., LECOEUR-TAIBI I., et al. | ||
|
2025A&A...700A.187U |
19 | D | 1 | 3121 | ~ | A population analysis of Galactic Miras with light-curve asymmetries. | UTTENTHALER S. and MERCHAN-BENITEZ P. |