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| NAME V1062 Sco Moving Group , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST12:02:32 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2018A&A...614A..81R | 1485 | S X C | 35 | 77 | 8 | A new compact young moving group around V1062 Scorpii. | ROSER S., SCHILBACH E., GOLDMAN B., et al. | ||
|
2020AJ....160..186L |
370 | X C | 8 | 235 | 15 | A Gaia survey for young stars associated with the Lupus clouds. | LUHMAN K.L. | ||
|
2021ApJ...917...23K |
685 | D | X C | 16 | 90 | 57 | Stars with photometrically young Gaia luminosities around the solar system (SPYGLASS). I. Mapping Young stellar structures and their star formation histories. | KERR R.M.P., RIZZUTO A.C., KRAUS A.L., et al. | |
|
2022AJ....163...24L |
1831 | A | D | X C | 43 | 14 | 18 | A census of the stellar populations in the Sco-Cen complex. | LUHMAN K.L. |
|
2022AJ....163...25L |
383 | X | 9 | 60 | 12 | A census of the circumstellar disk populations in the Sco-Cen complex. | LUHMAN K.L. | ||
|
2022AJ....163...26L |
213 | X C | 4 | 16 | 2 | Spectroscopy of candidate members of the Sco-Cen complex. | LUHMAN K.L. and ESPLIN T.L. | ||
|
2023A&A...677A..59R |
975 | D | X C | 22 | 13197 | ~ | Significance mode analysis (SigMA) for hierarchical structures An application to the Sco-Cen OB association. | RATZENBOCK S., GROSSSCHEDL J.E., MOLLER T., et al. | |
| 2023A&A...680A..39S | 522 | A | D | X C | 12 | 21 | ~ | Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble II. Advanced modelling of interstellar 26Al, 53Mn, 60Fe, and 244Pu influxes as traces of past supernova activity in the solar neighbourhood. | SCHULREICH M.M., FEIGE J. and BREITSCHWERDT D. |
| 2025ApJ...994..248F | 373 | X C | 7 | 16 | ~ | A Comprehensive Gaia Spectroscopic Study of Stars in the Scorpius-Centaurus Complex: Star Formation History and Disk Lifetime. | FANG M. and HERCZEG G.J. |