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| NAME Serpens-Aquila Complex , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST17:27:53 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
2019ApJ...878..111H 
|
447 | X C | 10 | 3863 | 48 | An initial overview of the extent and structure of recent star formation within the Serpens Molecular Cloud using Gaia Data Release 2. | HERCZEG G.J., KUHN M.A., ZHOU X., et al. | ||
| 2019A&A...628A..97C | 41 | X | 1 | 13 | ~ | Silicate features in the circumstellar envelopes of the Class I binary driving source of HH 250. | COMERON F., MERIN B., REIPURTH B., et al. | ||
| 2020ApJ...900..155Z | 41 | X | 1 | 6 | ~ | Molecular clouds surrounding supernova remnant G43.9+1.6: associated and nonassociated. | ZHOU X., SU Y., YANG J., et al. | ||
|
2022ApJ...925...39T
|
43 | X | 1 | 405 | 20 | The VLA/ALMA Nascent Disk And Multiplicity (VANDAM) Survey of Orion Protostars. V. A Characterization of Protostellar Multiplicity. | TOBIN J.J., OFFNER S.S.R., KRATTER K.M., et al. | ||
| 2022ApJ...941..135S | 43 | X | 1 | 21 | ~ | Herschel Optimized Tau and Temperature (HOTT) Maps: Uncertainty Analysis and Robust Parameter Extraction. | SINGH A. and MARTIN P.G. | ||
| 2023ApJ...944..226D | 44 | X | 1 | 8 | ~ | Near-infrared Polarimetry and H2 Emission toward Massive Young Stars: Discovery of a Bipolar Outflow Associated to S235 e2s3. | DEVARAJ R., CARATTI O GARATTI A., DEWANGAN L.K., et al. | ||
| 2024ApJ...966...91L | 45 | X | 1 | 44 | ~ | New Insights on the Accretion Properties of Class 0 Protostars from 2 μm Spectroscopy. | LE GOUELLEC V.J.M., GREENE T.P., HILLENBRAND L.A., et al. | ||
| 2024ApJ...967L..27L | 90 | X | 2 | 12 | ~ | Morphological Evidence for the eROSITA Bubbles Being Giant and Distant Structures. | LIU T., MERLONI A., SANDERS J., et al. | ||
| 2024ApJ...974..265K | 45 | X | 1 | 5 | ~ | Instability and Evolution of Shocked Clouds Formed by Orthogonal Collisions between Magnetized Filamentary Molecular Clouds. | KASHIWAGI R., IWASAKI K. and TOMISAKA K. |
