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| V* RY Tel , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST01:26:40 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1954ApJS....1..175B | 688 | 185 | Catalogue and bibliography of emission-line stars of types later than B. | BIDELMAN W.P. | |||||
|
1978MSS...C02....0H |
14 | D | 1 | 30388 | ~ | Catalogue of two dimentional spectral types for the HD stars, Vol. 2 | HOUK N. | ||
|
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. | |||
|
1993yCat.3135....0C |
14 | D | 1 | 252979 | 52 | VizieR Online Data Catalog: Henry Draper Catalogue and Extension, published in Ann. Harvard Obs. 91-100 (1918-1925) | CANNON A.J. and PICKERING E.C. | ||
|
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. |