GIARPS/GRAVITY Survey: Broad-Band 0.44–2.4 Micron High-Resolution Spectra of T-Tauri and Herbig AeBe Stars – Combining High Spatial and High Spectral Resolution Data to Unveil the Inner Disc Physics
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|Title:||GIARPS/GRAVITY Survey: Broad-Band 0.44–2.4 Micron High-Resolution Spectra of T-Tauri and Herbig AeBe Stars – Combining High Spatial and High Spectral Resolution Data to Unveil the Inner Disc Physics||Authors:||Massi, F.; Caratti o Garatti, Alessio; Garcia Lopez, R.; Coffey, Deirdre; et al.||Permanent link:||http://hdl.handle.net/10197/11158||Date:||2-Aug-2019||Online since:||2019-10-17T15:14:23Z||Abstract:||The GIARPS/GRAVITY survey aims to obtain a set of high spatial and spectral resolution data for a sample of T-Tauri and Herbig AeBe stars (∼100 objects) selected from the VLTI/GRAVITY GTO sample of Young Stellar Objects (YSOs). GIARPS is a broad-band spectrometer combining HARPS-N and GIANO which allows high-resolution spectra from 0.44 μm (R ∼ 115, 000) to 2.44 μm (R ∼ 50, 000) in one observation. By combining this high spectral resolution with the high spatial resolution (∼1 mas) of GRAVITY, a view of unprecedented detail can be obtained of the innermost regions of circumstellar discs in YSOs spanning a wide range of masses (0.1–5 M⊙) and ages (105–107 yr). The ultimate goal is to model the accretion and ejection mechanisms, and study how they evolve as a function of YSO mass and age, using the spatially and spectrally resolved atomic and molecular lines from the inner gaseous regions.||Type of material:||Conference Publication||Publisher:||Springer||Series/Report no.:||Astrophysics and Space Science Proceedings book series (ASSSP, volume 55)||Copyright (published version):||2019 Springer||DOI:||10.1007/978-3-030-14128-8_19||Language:||en||Status of Item:||Peer reviewed||Is part of:||Saulty, C. JET Simulations, Experiments and Theory: Ten Years After JETSET. What is Next?||ISBN:||9783030141271|
|Appears in Collections:||Physics Research Collection|
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