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| V* V1870 Ori , the SIMBAD biblio (22 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST07:13:13 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1996A&AS..119....7A | 164 | 117 | New weak-line T Tauri stars in Orion from the ROSAT all-sky survey. | ALCALA J.M., TERRANEGRA L., WICHMANN R., et al. | |||||
| 2000A&A...353..186A | 123 | 54 | High-resolution spectroscopy of ROSAT low-mass pre-main sequence stars in Orion. | ALCALA J.M., COVINO E., TORRES G., et al. | |||||
|
2005A&A...438..769D |
1380 | 87 | Pre-main sequence star Proper Motion Catalogue. | DUCOURANT C., TEIXEIRA R., PERIE J.-P., et al. | |||||
| 2005MmSAI..76..358M | 22 | 1 | Rotational periods of solar-mass WTTS in Orion. | MARILLI E., FRASCA A., ALCALA J.M., et al. | |||||
| 2007A&A...463.1081M | O | 49 | 15 | Rotational periods of solar-mass young stars in Orion. | MARILLI E., FRASCA A., COVINO E., 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. | ||
|
2011IBVS.5969....1K |
15 | D | 1 | 2041 | 27 | The 80th name-list of variable stars. Part I - RA 0h to 6h. | KAZAROVETS E.V., SAMUS N.N., DURLEVICH O.V., et al. | ||
|
2012A&A...548A..79A |
15 | D | 1 | 5274 | 86 | The first INTEGRAL-OMC catalogue of optically variable sources. | ALFONSO-GARZON J., DOMINGO A., MAS-HESSE J.M., et al. | ||
|
2018AJ....156...84K |
16 | D | 1 | 9041 | 228 | The APOGEE-2 survey of the Orion star-forming Complex. II. Six-dimensional structure. | KOUNKEL M., COVEY K., SUAREZ G., et al. | ||
|
2019AJ....157..196K |
16 | D | 1 | 12851 | 76 | Close companions around young stars. | KOUNKEL M., COVEY K., MOE M., 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. | ||
|
2019A&A...631A.166K |
16 | D | 1 | 1542 | 3 | Discovery of a 21 Myr old stellar population in the Orion complex. | KOS J., BLAND-HAWTHORN J., ASPLUND M., et al. | ||
|
2020AJ....160..120J |
16 | D | 1 | 365763 | 238 | APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. | JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al. | ||
|
2020ApJ...903...55P |
16 | D | 1 | 12301 | 12 | Open cluster chemical homogeneity throughout the Milky Way. | POOVELIL V.J., ZASOWSKI G., HASSELQUIST S., et al. | ||
|
2021MNRAS.506..150B |
17 | D | 1 | 588596 | 276 | The GALAH+ survey: Third data release. | BUDER S., SHARMA S., KOS J., et al. | ||
|
2021ApJ...923..177S |
17 | D | 1 | 9744 | 13 | Stellar rotation of T Tauri stars in the Orion Star-forming Complex. | SERNA J., HERNANDEZ J., KOUNKEL M., et al. | ||
|
2022AJ....163..152S |
17 | D | 1 | 583193 | 11 | APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. | SPRAGUE D., CULHANE C., KOUNKEL M., et al. | ||
|
2022ApJS..259...35A |
17 | D | 1 | 611005 | 320 | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. | ABDURRO'UF, ACCETTA K., AERTS C., et al. | ||
|
2022ApJ...931..156P |
17 | D | 1 | 22106 | 16 | 3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR 3. II. Hierarchical Star Formation Revealed by Spatial and Kinematic Substructures. | PANG X., TANG S.-Y., LI Y., et al. | ||
|
2022ApJS..262....7H |
17 | D | 1 | 134735 | 19 | A Blind All-sky Search for Star Clusters in Gaia EDR3: 886 Clusters within 1.2 kpc of the Sun. | HE Z., WANG K., LUO Y., et al. | ||
|
2023AJ....165...51R |
17 | D | 1 | 3791 | 3 | Stellar Properties for a Comprehensive Collection of Star-forming Regions in the SDSS APOGEE-2 Survey. | ROMAN-ZUNIGA C.G., KOUNKEL M., HERNANDEZ J., et al. | ||
|
2023ApJS..265...12Q |
17 | D | 1 | 58898 | 5 | Hunting for Neighboring Open Clusters with Gaia DR3: 101 New Open Clusters within 500 pc. | QIN S., ZHONG J., TANG T., et al. |