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TYC 71-542-1 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST17:18:55 |
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 |
---|---|---|---|---|---|---|---|---|---|
1997A&A...325..613F | 133 | 52 | New proper motions of pre-main sequence stars in Taurus-Auriga. | FRINK S., ROESER S., NEUHAEUSER R., et al. | |||||
1997A&A...325..647N | 125 | 76 | Optical high-resolution spectroscopy of ROSAT detected late-type stars south of the Taurus molecular clouds. | NEUHAEUSER R., TORRES G., STERZIK M.F., et al. | |||||
1997A&AS..124..449M | 140 | 58 | Search for young low-mass stars in a ROSAT selected sample south of the Taurus-Auriga molecular clouds. | MAGAZZU A., MARTIN E.L., STERZIK M.F., et al. | |||||
1997AJ....114.1555S | 111 | 8 | Binary search among X-ray active stars south of the Taurus molecular cloud. | STERZIK M.F., DURISEN R.H., BRANDNER W., et al. | |||||
1999A&A...346..878M | 87 | 6 | Radio emission from RASS sources south of Taurus-Auriga. | MAGAZZU A., UMANA G. and MARTIN E.L. | |||||
2005A&A...438..769D | 1380 | 87 | Pre-main sequence star Proper Motion Catalogue. | DUCOURANT C., TEIXEIRA R., PERIE J.-P., et al. | |||||
2010ApJ...723.1542X | 15 | D | 1 | 128 | 12 | Lithium abundances from optical high-resolution spectroscopy of weak-line T Tauri stars. | XING L.F. | ||
2019AJ....157...78J | 17 | D | 1 | 11564 | 44 | A catalog of wide binary and multiple systems of bright stars from Gaia-DR2 and the Virtual Observatory. | JIMENEZ-ESTEBAN F.M., SOLANO E. and RODRIGO C. | ||
2019MNRAS.490.3158C | 17 | D | 1 | 465834 | 28 | A catalogue of stellar diameters and fluxes for mid-infrared interferometry. | CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al. | ||
2020AJ....159..105L | 17 | D | 3 | 158 | ~ | Discovery of two nearby post-T Tauri stellar associations. | LIU J., FANG M. and LIU C. | ||
2020ApJ...903...96G | 17 | D | 4 | 588 | 27 | The µ Tau Association: a 60 Myr old coeval group at 150 pc from the Sun. | GAGNE J., DAVID T.J., MAMAJEK E.E., et al. |