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| [LSY2018] G350.54+00.69 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST22:25:00 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2018MNRAS.478.2119L | 385 | T A | X | 9 | 36 | 5 |
The straight and isolated G350.54+0.69 filament: density profile and star formation content. |
LIU H.-L., STUTZ A. and YUAN J.-H. | |
| 2019MNRAS.487.1259L | 1486 | T K A | X C F | 34 | 16 | ~ |
Large-scale periodic velocity oscillation in the filamentary cloud G350.54+0.69. |
LIU H.-L., STUTZ A. and YUAN J.-H. | |
| 2020A&A...635A.188L | 41 | X | 1 | 10 | ~ | Physical and chemical modeling of the starless core L 1512. | LIN S.-J., PAGANI L., LAI S.-P., et al. | ||
| 2021MNRAS.500.2831W | 42 | X | 1 | 15 | ~ | Striations, integrals, hourglasses, and collapse - thermal instability driven magnetic simulations of molecular clouds. | WAREING C.J., PITTARD J.M. and FALLE S.A.E.G. | ||
| 2021MNRAS.506.6081D | 42 | X | 1 | 15 | 3 | Lynds Bright Nebulae: sites of possible twisted filaments and ongoing star formation. | DEWANGAN L.K., DHANYA J.S., BHADARI N.K., et al. | ||
|
2022ApJS..259...36G |
43 | X | 1 | 13 | 4 | A Census of 163 Large-scale (>=10 pc), Velocity-coherent Filaments in the Inner Galactic Plane: Physical Properties, Dense-gas Fraction, and Association with Spiral Arms. | GE Y. and WANG K. | ||
|
2023RAA....23a5019S |
44 | X | 1 | 20 | ~ | Large-scale CO (J = 1-0) Observations toward the M120.1+3.0 Molecular Cloud: A Filament with a Chain of Starburst Clusters. | SUN L., CHEN X., FENG J., et al. | ||
| 2023ApJ...946...22D | 44 | X | 1 | 10 | 2 | IC 5146 Dark Streamer: The First Reliable Candidate of Edge Collapse, Hub-filament Systems, and Intertwined Sub-filaments. | DEWANGAN L.K., BHADARI N.K., MEN'SHCHIKOV A., et al. | ||
| 2023ApJ...957...61H | 44 | X | 1 | 9 | ~ | Investigating the Globally Collapsing Hub-Filament Cloud G326.611+0.811. | HE Y.-X., LIU H.-L., TANG X.-D., et al. |