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| [LH98] 168 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST00:35:00 |
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trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
1998A&AS..132..173L 
|
177 | 42 | Newly discovered candidate weak-line T Tauri stars in the surrounding area of the Taurus-Auriga region. | LI J.Z. and HU J.Y. | |||||
|
2005A&A...438..769D
|
1380 | 87 | Pre-main sequence star Proper Motion Catalogue. | DUCOURANT C., TEIXEIRA R., PERIE J.-P., et al. | |||||
|
2009ApJS..184..138H
|
15 | D | 2 | 20667 | 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. | ||
|
2014ApJ...784..126E
|
16 | D | 1 | 1466 | 39 | A WISE survey of circumstellar disks in Taurus. | ESPLIN T.L., LUHMAN K.L. and MAMAJEK E.E. | ||
|
2017ApJ...838..150K
|
16 | D | 1 | 421 | 70 | The greater Taurus-Auriga ecosystem. I. There is a distributed older population. | KRAUS A.L., HERCZEG G.J., RIZZUTO A.C., et al. | ||
|
2017AJ....154..134E
|
382 | D | X C | 9 | 483 | 15 | A survey for planetary-mass brown dwarfs in the Taurus and Perseus star-forming regions. | ESPLIN T.L. and LUHMAN K.L. | |
|
2018AJ....156..271L
|
99 | D | X | 3 | 630 | 108 | The stellar membership of the Taurus star-forming region. | LUHMAN K.L. | |
|
2019AJ....158...54E
|
100 | D | X | 3 | 633 | 47 | A survey for new members of Taurus from stellar to planetary masses. | ESPLIN T.L. and LUHMAN K.L. | |
|
2021AJ....162..110K
|
17 | D | 1 | 605 | 44 | Gaia EDR3 reveals the substructure and complicated star formation history of the greater Taurus-Auriga star-forming complex. | KROLIKOWSKI D.M., KRAUS A.L. and RIZZUTO A.C. | ||
|
2021ApJ...920..132P
|
17 | D | 1 | 5441 | 33 | Quantifying variability of young stellar objects in the mid-infrared over 6 years with the Near-Earth Object Wide-field Infrared Survey Explorer. | PARK W., LEE J.-E., CONTRERAS PENA C., et al. |
