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| V* V909 Car , the SIMBAD biblio (19 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST08:35:21 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2006A&A...460..695T |
15 | D | 1891 | 534 | Search for associations containing young stars (SACY). I. Sample and searching method. | TORRES C.A.O., QUAST G.R., DA SILVA L., et al. | |||
|
2009A&A...503.1023F |
68 | 1 | A variability sample catalogue selected from the Sydney observatory galactic survey. | FRESNEAU A. and OSBORN W.H. | |||||
|
2009ApJS..184..138H |
15 | D | 2 | 20623 | 68 | XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. | HAAKONSEN C.B. and RUTLEDGE R.E. | ||
|
2014A&A...568A..26E |
15 | D | 1 | 270 | 46 | Search for associations containing young stars (SACY). V. Is multiplicity universal? Tight multiple systems. | ELLIOTT P., BAYO A., MELO C.H.F., et al. | ||
|
2015A&A...580A..88E |
16 | D | 1 | 219 | 21 | Search for associations containing young stars (SACY). VI. Is multiplicity universal? Stellar multiplicity in the range 3-1000 au from adaptive-optics observations. | ELLIOTT P., HUELAMO N., BOUY H., et al. | ||
|
2016A&A...590A..13E |
16 | D | 2 | 646 | 29 | Search for associations containing young stars (SACY). VII. New stellar and substellar candidate members in the young associations. | ELLIOTT P., BAYO A., MELO C.H.F., et al. | ||
|
2017AJ....153...75K |
16 | D | 1 | 451448 | 394 | The Radial Velocity Experiment (RAVE): fifth data release. | KUNDER A., KORDOPATIS G., STEINMETZ M., et al. | ||
|
2014ASPC..485..223B |
15 | D | 1 | 465820 | 45 | The JMMC stellar diameters catalog v2 (JSDC): a new release based on SearchCal improvements | BOURGES L., LAFRASSE S., MELLA G., et al. | ||
|
2018A&A...609A.116R |
16 | D | 1 | 143018 | 65 | Empirical photometric calibration of the Gaia red clump: Colours, effective temperature, and absolute magnitude. | RUIZ-DERN L., BABUSIAUX C., ARENOU F., et al. | ||
|
2018A&A...615A..49C |
16 | D | 1 | 224763 | 54 | Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution. | CANTAT-GAUDIN T., VALLENARI A., SORDO R., et al. | ||
|
2018ApJ...867...93R |
16 | D | 2 | 345 | ~ | Kinematic identification of young nearby moving groups from a sample of chromospherically active stars in the RAVE catalog. | RAMIREZ-PRECIADO V.G., ROMAN-ZUNIGA C.G., AGUILAR L., et al. | ||
|
2019AJ....158..122K |
16 | D | 1 | 290057 | 150 | Untangling the Galaxy. I. Local structure and star formation history of the Milky Way. | KOUNKEL M. and COVEY K. | ||
|
2019MNRAS.490.3158C |
16 | D | 1 | 465839 | 28 | A catalogue of stellar diameters and fluxes for mid-infrared interferometry. | CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al. | ||
|
2020ApJ...890...46T |
16 | D | 1 | 403 | 45 | Superflares on solar-type stars from the first year observation of TESS. | TU Z.-L., YANG M., ZHANG Z.J., et al. | ||
|
2020MNRAS.494.3596D |
16 | D | 1 | 211 | 32 | Superflares and variability in solar-type stars with TESS in the Southern hemisphere. | DOYLE L., RAMSAY G. and DOYLE J.G. | ||
|
2020AJ....160...83S |
16 | D | 1 | 451375 | 83 | The sixth Data Release of the Radial Velocity Experiment (RAVE). II. Stellar atmospheric parameters, chemical abundances, and distances. | STEINMETZ M., GUIGLION G., McMILLAN P.J., et al. | ||
|
2021A&A...645A..30Z |
17 | D | 2 | 431 | 20 | Search for associations containing young stars (SACY). VIII. An updated census of spectroscopic binary systems exhibiting hints of non-universal multiplicity among their associations. | ZUNIGA-FERNANDEZ S., BAYO A., ELLIOTT P., et al. | ||
|
2022ApJ...928...70C |
17 | D | 1 | 5007 | 6 | Pearls on a String: Numerous Stellar Clusters Strung Along the Same Orbit. | CORONADO J., FURNKRANZ V. and RIX H.-W. | ||
|
2024AJ....167..210V |
18 | D | 1 | 7289 | ~ | The Occurrence of Small, Short-period Planets Younger than 200 Myr with TESS. | VACH S., ZHOU G., HUANG C.X., et al. |