LAMOST reveals secret of stellar rotation of hot stars

LAMOST reveals secret of stellar rotation of hot stars
Figure 1. Normalized sample spectra, in the rest frame, from LAMOST MRS DR7 (blue) and the corresponding best-fitting models (orange) determined by the SLAM algorithm (see Section 3). Blue and red segments of the same object are shown in the left and right panels, respectively. The best-fitting effective temperatures, Teff, and the projected rotational velocities, v sin i, are listed in the bottom right corners. The red bands correspond to the spectral regions covering Mg i b (5160.12–5192.62 Å) and Hα (6548.0–6578.0 Å). Credit: DOI: 10.3847/1538-4365/ac1acf

Stars all rotate, but at different rates. Stellar rotation profoundly affects almost every aspect of stellar evolution. But the evolution of the angular momentum remains a mystery.

A new study led by Ph.D. candidate Sun Weijia from Peking University and the National Astronomical Observatories of Chinese Academy of Sciences (NAOC) provides a fresh comprehension of their rotation behavior by studying the rotational velocity of hundreds of thousands of massive .

Related results were published in The Astrophysical Journal Supplement Series and The Astrophysical Journal.

The Sun has a mean rotational velocity of about 2 km/s at its equator, while more massive stars can reach a rotational velocity of hundreds of km/s. Such a vast difference poses fundamental questions about the origin and the of these fast rotators' angular momentum.

"Fast rotation is ubiquitous among massive stars," said Sun Weijia, the leading author of this series of studies. "Our study provides clues for understanding how the angular momentum of massive stars evolves during the majority of its lifetime."

To investigate their rotational behavior, the researchers used from the latest survey based on the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), which is spectroscopically observing tens of millions of stars.

By using a novel data-driven method, they obtained the stellar properties of over 40,000 , which paves the way for reviewing the properties of stellar rotation distributions to unprecedented accuracy and details.

"Such a catalog will reform our understanding of massive star evolution," he said. "Our data challenges the idea that stars with peculiar chemical abundance are all slow rotators."

Moreover, these works reveal the detailed structure of how rotation rates vary as a function of stellar mass and metallicity.

The complicated rotation map reveals the inner environment of hot stars, composed of radiative envelop and convective core. Its dependence on metallicity will help us understand the chemical enrichment history of our Milky Way and the contribution of rotation on the oldest stars in the cosmos.


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More information: Weijia Sun et al, Exploring the Stellar Rotation of Early-type Stars in the LAMOST Medium-resolution Survey. I. Catalog, The Astrophysical Journal Supplement Series (2021). DOI: 10.3847/1538-4365/ac1acf

Weijia Sun et al, Exploring the Stellar Rotation of Early-type Stars in the LAMOST Medium-resolution Survey. II. Statistics, The Astrophysical Journal (2021). DOI: 10.3847/1538-4357/ac1ad0

Journal information: Astrophysical Journal

Citation: LAMOST reveals secret of stellar rotation of hot stars (2022, January 21) retrieved 26 May 2022 from https://phys.org/news/2022-01-lamost-reveals-secret-stellar-rotation.html
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