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Researchers detect a new molecular bubble–outflow structure

Researchers detect a new molecular bubble-outflow structure
The position, multi-wavelength images, and spectra of the molecular bubble. The upper right panels are the images of 12CO, 13CO, C18O, and 250 μm continum. The lower right panels show the average spectra of the molecular bubble (dotted line) and the outflow (solid line). Credit: Duan Yan

The process of star formation interacts with the surrounding environment and produces observable dynamical phenomena, such as outflows and bubbles, collectively known as stellar feedbacks. As one of the primary sources of energy injection into the natal cloud, such feedbacks are critical for the evolution of interstellar medium.

An international team led by Dr. Li Di from the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC) conducted carbon-monoxide emission observations in the Taurus molecular clouds using the Institute for Radio Astronomy in the Millimeter Range (IRAM) 30-m telescope and James Clerk Maxwell Telescope (JCMT). They identified a new molecular bubble in the carbon monoxide signal from both telescopes.

The study was published in The Astrophysical Journal on Feb. 7.

"Through combined analysis with the Five College Radio Astronomy Observatory (FCRAO) survey of the Taurus molecular cloud, we found an outflow located at the center of the molecular bubble," said Duan Yan, a Ph.D. candidate from NAOC and the first author of the study.

Based on Gaia EDR3 data, the researchers suggested that a pair of T Tauri might have produced the molecular bubble 70,000 years ago. Only one similar case of a molecular bubble coexisting with an outflow (in Orion A) has been reported before.

This discovery supports the common origin of molecular and outflows. It enhances our understanding of how stellar feedback acts on . The detection of the bubble–outflow structure provides new observational evidence for the feedbacks of T Tauri stars to the interstellar medium.

Dr. Paul F. Goldsmith from Jet Propulsion Laboratory and Dr. Laurent Pagani from Observatoire de Paris contributed to the estimation of physical parameters and the driving-source analysis of the molecular bubble- structure.

More information: Yan Duan et al, Discovery of a New Molecular Bubble–Outflow Structure in the Taurus B18 Cloud, The Astrophysical Journal (2023). DOI: 10.3847/1538-4357/aca805

Journal information: Astrophysical Journal

Citation: Researchers detect a new molecular bubble–outflow structure (2023, February 8) retrieved 21 July 2024 from
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