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| V* GK Mon , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST05:20:43 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1933AN....249..383M | 22 | 3 | 21 neue Veranderliche. | MORGENROTH O. | |||||
| 1975AJ.....80..515R | 35 | 88 | Preeruption light curves of novae. | ROBINSON E.L. | |||||
|
1988IRASP.C......0J |
14 | D | 1 | 245223 | ~ | Infrared Astronomical Satellite Catalogs, 1988. The Point Source Catalog, version 2.0, NASA RP-1190 | JOINT IRAS SCIENCE WORKING GROUP | ||
|
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. | |||
|
2004AJ....128.2965W |
15 | D | 1 | 8686 | 106 | Identifying red variables in the Northern Sky Variability Survey. | WOZNIAK S.J., WILLIAMS P.R., VESTRAND W.T., et al. | ||
| 2004BAVSR..53..145R | 46 | 0 | Aus der Sektion 'Karten". Neues aus der AAVSO zum Thema Umgebungskarten ! | RATZ K. | |||||
|
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. | ||
|
2017ARep...61...80S |
16 | D | 7150 | 446 | General catalogue of variable stars: Version GCVS 5.1 | SAMUS N.N., KAZAROVETS E.V., DURLEVICH O.V., et al. | |||
|
2019MNRAS.486.1907J |
16 | D | 1 | 8966 | 183 | The ASAS-SN catalogue of variable stars - II. Uniform classification of 412 000 known variables. | JAYASINGHE T., STANEK K.Z., KOCHANEK C.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. |