The emergence of molecular complexity in star forming regions as seen with ASAI

Abstract

The Large Program "Astrochemical Surveys At IRAM" (ASAI) investigates the emergence of molecular complexity along the different stages of the solar-type star formation process, by carrying out unbiased line surveys of a sample of ten template sources in the range 80-272 GHz with the IRAM 30m telescope. We present here an overview of the main results of the Large Program ASAI.

6 pages, 4 figures; invited talk at the IRAM conference "Multi-line Diagnostics of the Interstellar Medium", Nice, April 2022; To be published in The European Physical Journal Web of Conferences

References in corpus (12)

• Complex Chemistry in Star-Forming Regions: An Expanded Gas-Grain Warm-up Chemical Model
• The origin of complex organic molecules in prestellar cores
• The Spatial Distribution of Complex Organic Molecules in the L1544 Pre-stellar Core
• Formation of Complex Molecules in Prestellar Cores: a Multilayer Approach
• Shedding light on the formation of the pre-biotic molecule formamide with ASAI
• Seeds of Life in Space (SOLIS) III. Formamide in protostellar shocks: evidence for gas-phase formation
• Molecules with a peptide link in protostellar shocks: a comprehensive study of L1157
• Interstellar formamide (NH${}_2$CHO), a key prebiotic precursor
• Decrease of the organic deuteration during the evolution of Sun-like protostars: the case of SVS13-A
• Detection of the HC${}_3$NH${}^{+}$ and HCNH${}^{+}$ ions in the L1544 pre-stellar core
• Isocyanogen formation in the cold interstellar medium
• Hot and dense water in the inner 25 AU of SVS13-A