This stream of gas transports material from the clouds surrounding the star-forming area within Perseus directly into an emerging binary star system known as SVS 13A.
Stars are formed from clouds of gas and dust, and recent observations indicate that the process of star formation is far more dynamic than previously understood.
New findings from the Atacama Large Millimeter/Submillimeter Array (ALMA) reveal both dust and molecules swirling around the SVS 13A system. This data shows how the magnetic field not only permeates these stellar nurseries but actively directs the flow of matter, offering a preferred path for gas to accumulate in the disk where new stars and planets arise.
“Visualize a garden hose, but instead of water, it smoothly channels materials for star formation through intricate pathways carved by unseen forces,” explains Dr. Paulo Cortes, an astronomer at the NSF National Radio Astronomy Observatory and the joint ALMA telescope.
“This perspective from ALMA observations presents channels of gas known as subalfvénic streamers, regulated by spiral magnetic field lines.”
“This new data provides an insightful glimpse into the star formation process.”
“These streamers illustrate how magnetic fields can influence star formation by managing material influx, akin to a private highway facilitating car travel.”
ALMA’s images and findings uncover two spiral arms of dust encircling the star, with gas streams closely mirroring the same trajectory.
This remarkable configuration implies that the gas within the streamer is traversing at a slower pace than previously believed, reinforcing the concept of a magnetized channel rather than a chaotic, collapsing cloud.
The presence of such streamers, linking clouds to disks and supplying them with material in a managed fashion, indicates that both gravity and magnetism are crucial in the formation of stars and the shaping of potential planetary bodies around them.
This groundbreaking result signifies the first instance where astronomers have directly mapped both a streamer and its associated magnetic field in a single observation.
“Subalfvenic streamers indicate a fresh role for magnetic fields amidst gravitational dominance, acting as ‘guides’ to assist the descent of material from the outer envelope to the disk,” the astronomers remarked.
Upcoming findings are detailed in a paper in the Astrophysics Journal Letter.
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PC Cortez et al. 2025. First results from ALPPS: SVS 13A subalfvenic streamer. APJL 992, L31; doi: 10.3847/2041-8213/ae0c04
Source: www.sci.news
