Cooling Process of the High-mass Young Stellar Object G24.33+0.14 Following an Accretion Burst
The high-mass young stellar object G24.33+0.14 (G24), has recently been observed to undergo an accretion burst since 2019 September, lasting approximately two years. By utilizing 1.3 mm observational data from the NOrthern Extended Millimeter Array in 2020 March and the Atacama Large Millimeter/subm...
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| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
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| Series: | The Astronomical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-3881/adc928 |
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