Discovery of Radio Recombination Lines from Proplyds in the Orion Nebula Cluster

Discovery of Radio Recombination Lines from Proplyds in the Orion Nebula Cluster

We present new Atacama Large Millimeter/submillimeter Array observations that, for the first time, detect hydrogen and helium radio recombination lines from a protoplanetary disk. We imaged the Orion Nebula Cluster at 3.1 mm with a spectral setup that covered the n = 42 → 41 transitions of hydrogen...

Full description

Saved in:
Bibliographic Details
Main Authors: Ryan D. Boyden, Kimberly L. Emig, Nicholas P. Ballering, Charles J. Law, Thomas J. Haworth, Jonathan C. Tan, L. Ilsedore Cleeves, Zhi-Yun Li
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Proplyds
Protoplanetary disks
Planet formation
Photoionization
Submillimeter astronomy
Radio astronomy
Online Access:https://doi.org/10.3847/1538-4357/adbbcc
Tags: Add Tag
No Tags, Be the first to tag this record!

Internet

https://doi.org/10.3847/1538-4357/adbbcc

Similar Items