New Ways Developed to See the Formation of Stars in the Milky Way
A research team led by Adler Planetarium astronomer Dr. Grace Wolf-Chase has discovered new evidence of stars forming in our Milky Way Galaxy. By using a telescope equipped to detect infrared light invisible to our eyes, this exciting new science is revealing how stars, including our very own Sun, grow up within clusters and groups. The Astrophysical Journal has published a paper on the subject titled, “MHOs Toward HMOs: A Search for Molecular Hydrogen Emission-Line Objects Toward High-Mass Outflows.”
The team found huge gas clouds moving outward from areas where “baby” stars are forming, using a new way of disentangling these outflows from other processes in densely-populated stellar nurseries. These stellar nurseries can produce dozens or even hundreds of stars with different sizes and masses.
“The Sun, though isolated from other stars today, is thought to have formed in a cluster with many other stars, so the environments we’re studying can tell us a lot about the origin of our own solar system,” said Wolf-Chase.
Stars form when cold, rotating clouds of gas and dust in space are pulled together by gravity into flattened “disks” that spin faster as they shrink, similar to what happens when twirling figure skaters pull their outstretched arms in toward their bodies. In order for a star to form at the center of a spinning disk, the rotation of the disk must slow down. This happens through powerful outflows of gas that are channeled into tight streams, known as “jets.” Jets can span more than 10 trillion miles, even though the disks that launch them are “mere” billions of miles across (comparable to the size of our solar system). Since planets can form in the disks, the presence of a jet can be a good indicator of a nascent planetary system, even when the disk isn’t observed directly. Stars more than eight times as massive as the Sun bathe their surroundings in intense ultraviolet radiation that destroys their natal clouds quickly, so it’s not clear if these massive stars develop disks and jets similar to stars like the Sun.
The researchers used an instrument called NICFPS (which stands for Near-Infrared Camera and Fabry-Perot Spectrometer) on the Astrophysical Research Consortium (ARC) 3.5-meter telescope at the Apache Point Observatory (APO) in Sunspot, New Mexico. NICFPS peered into 26 dusty clouds thought to be forming clusters containing massive stars. Using a combination of infrared filters that allowed them to distinguish jets from infant stars from other types of light produced by the radiation in these massive stellar nurseries, they identified 36 jets across 22 of the regions. These results provide compelling evidence that, like their lower-mass siblings, massive stars also launch powerful jets. The jet shuts off shortly after radiation from the massive star begins to disrupt its environment.
Reference:
“MHOs Toward HMOs: A Search for Molecular Hydrogen Emission-line Objects Toward High-Mass Outflows,” G. Wolf-Chase, K. Arvidsson & M. Smutko, 2017 July 20 [http://iopscience.iop.org/article/10.3847/1538-4357/aa762a, preprint: https://arxiv.org/abs/1706.00375]. Grace Wolf-Chase, an Astronomer at the Adler Planetarium, is first author of this paper. Co-authors are former Postdoctoral Scholar at the Adler Planetarium, Kim Arvidsson, who is currently Assistant Professor of Physics in the Trull School of Sciences and Mathematics at Schreiner University in Kerrville, Texas; and Michael Smutko, Professor of Instruction in the Department of Physics and Astronomy at Northwestern University and former Astronomer at the Adler Planetarium. Astronomical research at the Adler Planetarium is funded in part through a generous grant from the Brinson Foundation. This project also received a Research Seed Grant through NASA’s Illinois Space Grant Consortium.
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