305 citations · 6.7k across the 125 of their papers we have counts for
125 papers
CHOH and HCN in Interstellar Comet 3I/ATLAS Mapped with the ALMA Atacama Compact Array: Distinct Outgassing Behaviors and a Remarkably High CHOH/HCN Production Rate Ratio
Nathan X. Roth, Martin A. Cordiner, Dominique Bockelée-Morvan +15
We report the detection of methanol (CHOH) toward interstellar comet 3I/ATLAS using the Atacama Compact Array of the Atacama Large Millimeter/Submillimeter Array (ALMA) on UT 2…
ALMAGAL VII. Cataloging Hierarchical Mass Structure from Cores to Clumps across the Galactic Disk
Jennifer Wallace, Taevis Kolz, Cara Battersby +42
Investigating the multi-scale fragmentation of dense clumps into compact cores is essential for understanding the processes that govern the initial distribution of mass in stellar…
JWST ice band profiles reveal mixed ice compositions in the HH 48 NE disk
Jennifer B. Bergner, J. A. Sturm, Elettra L. Piacentino +19
Planet formation is strongly influenced by the composition and distribution of volatiles within protoplanetary disks. With JWST, it is now possible to obtain direct observational c…
Mapping Physical Conditions in Neighboring Hot Cores: NOEMA Studies of W3(HO) and W3(OH)
Morgan M. Giese, Will E. Thompson, Dariusz C. Lis +1
The complex chemistry that occurs in star-forming regions can provide insight into the formation of prebiotic molecules at various evolutionary stages of star formation. To study t…
Retrievals of Protoplanetary Disk Parameters using Thermochemical Models: I. Disk Gas Mass from Hydrogen Deuteride Spectroscopy
Young Min Seo, Karen Willacy, Geoffrey Bryden +4
We discuss statistical relationships between the mass of protoplanetary disks and the hydrogen deuteride (HD) line emission and the dust spectral energy distribution (SED) determin…
Comparing Complex Chemistry in Neighboring Hot Cores: NOEMA Studies of W3(HO) and W3(OH)
Will E. Thompson, Morgan M. Giese, Dariusz C. Lis +1
Presented here are NOEMA interferometric observations of the neighboring hot cores W3(HO) and W3(OH). The presence of two star-forming cores at different evolutionary stages…