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- An astrophysical maser is a naturally occurring source of stimulated spectral line emission, typically in the microwave portion of the electromagnetic spectrum12. Maser emission is observed from the circumstellar envelopes of evolved stars, molecular clouds/star-forming regions, active galactic nuclei, supernova remnants, comets, and the Saturnian moons2. This emission may arise in molecular clouds, comets, planetary atmospheres, stellar atmospheres, or various other conditions in interstellar space1.Learn more:✕This summary was generated using AI based on multiple online sources. To view the original source information, use the "Learn more" links.An astrophysical maser is a naturally occurring source of stimulated spectral line emission, typically in the microwave portion of the electromagnetic spectrum. This emission may arise in molecular clouds, comets, planetary atmospheres, stellar atmospheres, or various other conditions in interstellar space.en.wikipedia.org/wiki/Astrophysical_maserAn astrophysical MASER (Microwave Amplification by Stimulated Emission of Radiation) is a source of stimulated spectral line emission. Maser emission is observed from the circumstellar envelopes of evolved stars, molecular clouds/star-forming regions, active galactic nuclei, supernova remnants, comets, and the Saturnian moons.arxiv.org/abs/1104.2306
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A maser is a device that produces coherent electromagnetic waves , through amplification by stimulated emission. The term is an acronym for microwave …
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Masers | Center for Astrophysics | Harvard
Identifying and studying astronomical masers around stars using the CfA Submillimeter Array (SMA) and other observatories. That includes discovering some of the first known naturally-occurring hydrogen masers, which are much …
astrophysics - How do we know that comets definitely …
Wikipedia's Astrophysical_maser#comets mentions some anecdotes of notable masers associated with comets, and Maser emissions from comets begins: The 18-cm lines of the OH radical are the only well-documented masers in comets.
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