Access the full text.
Sign up today, get DeepDyve free for 14 days.
[It has been established that the Universe consists of dark energy, dark matter, and baryons. Although the mass of baryons is only 4.6% of the total mass of the Universe, they form rich structures in the Universe from large scales (clusters of galaxies and galaxies) to small scales (stars and planets). Among such hierarchical structure, stars are the most fundamental physical elements in the Universe. They also play important roles in chemical evolution of the Universe through nucleosyntheses. All said and done, they harbor planets where the life can emerge. Thus, detailed understanding of star formation is a central issue for astrophysics and astrochemistry. This thesis describes a part of such efforts, focusing on a relation between physical and chemical processes of the star and planetary system formation.]
Published: Nov 9, 2022
Keywords: Star formation; Radio astronomy; Low-mass star; Protostellar disks; Protoplanetary disks; Jets and outflows; Interstellar medium; Astrochemsitry
Read and print from thousands of top scholarly journals.
Already have an account? Log in
Bookmark this article. You can see your Bookmarks on your DeepDyve Library.
To save an article, log in first, or sign up for a DeepDyve account if you don’t already have one.
Copy and paste the desired citation format or use the link below to download a file formatted for EndNote
Access the full text.
Sign up today, get DeepDyve free for 14 days.
All DeepDyve websites use cookies to improve your online experience. They were placed on your computer when you launched this website. You can change your cookie settings through your browser.