Astrophysical masers are microwave lasers that happen naturally in house. They’re present in areas of gasoline which were heated or compressed by shock waves. Due to this, astrophysical masers are sometimes present in molecular clouds close to forming stars, the place protostellar jets can collide with them and created shiny beams of microwave mild. Due to their depth, masers are a strong instrument for probing areas of gasoline the place shockwaves happen.
Ionized jet and water masers in IRAS 18553+0414. Credit score: Ananay Sethi.
Ananay Sethi, a graduate pupil at New Mexico Tech, has studied masers close to high-mass protostars to higher perceive their formation course of. To do that, Ananay used information gathered by the Very Giant Array (VLA) within the A configuration utilizing the Ok-band, which has a wavelength of round 1.3cm. He needed to see if maser emissions may very well be used to hint the alignment of jets from high-mass protostars. The observations of maser mild from water molecules confirmed that they had been brought on by ionized jets. Ananay’s preliminary outcomes additionally confirmed that the masers gave good outlines of the molecular outflows from high-mass protostar jets, suggesting they can be utilized to hint the circulation of those jets.
Ananay offered these outcomes at AAS242.
.jpg){kind=small}
