generous support of the Independent Innovation Project for Postgraduates of Central South University No.160171008;supported by the National Natural Science Foundation of China,and projects Nos.11803026,U2031204。
We have chosen the Large Scale Atomic/Molecular Massively Parallel Simulator (LAMMPS) code to calculate the coalescence of silicon carbide (SiC),silicon oxide dust (SiO) in the AGB stellar wind.LAMMPS is a classica mo...
the Independent Innovation Project for Postgraduates of Central South University(No.160171008);the National Natural Science Foundation of China(project No.U2031204);the project of Xinjiang(No.2021D01C075)。
Polycyclic aromatic hydrocarbons(PAHs),PANHs,and peptoids dust spectral calculations from the interstellar medium(ISM)are important for dust observations and theory.Our goal is to calculate the radiation spectrum of s...
supported by the National Natural Science Foundation of China(NSFC)through grant Nos.12133002,U2031209 and 12203025;Shandong Provincial Natural Science Foundation through project ZR2022QA064;the CSST Milky Way and Nearby Galaxies Survey on Dust and Extinction Project CMS-CSST2021-A09。
Dust extinction law is crucial to recover the intrinsic energy distribution of celestial objects and infer the characteristics of interstellar dust.Based on the traditional pair method,an improved pair method is propo...
The Guo Shou Jing Telescope(the Large-sky Area Multi-Object Fiber Spectroscopic Telescope,LAMOST)is a National Major Scientific Project built by the Chinese Academy of Sciences.Funding for the project has been provided by the National Development and Reform Commission;supported by the National Natural Science Foundation of China(NSFC,Grant No.12073047)。
Large scale spectroscopic surveys such as that using Large-sky Area Multi-Object Fiber Spectroscopic Telescope(LAMOST) have collected spectra of millions stars in the Milky Way.Utilizing this huge sample of stars to s...
supported by the National Natural Science Foundation of China(NSFC,Grant Nos.11988101,12090044,12090040,11673030,42075123 and 62127901);the National Key R&D Program of China under grant No.2019YFA0405502。
The Stellar Abundances and Galactic Evolution Survey(SAGES)is a multi-band photometric survey focused on estimation of stellar atmospheric parameters and interstellar extinction.In this paper we have derived photonic ...
The distribution of ultraviolet(UV)radiation field provides critical constraints on the physical environments of molecular clouds.Within 1 kpc of our solar system and fostering protostars of different masses,the giant...
the National Natural Science Foundation of China(Grant Nos.U1931209,12003050,11970360,12090044 and 12103068);the National Key R&D Program of China(Nos.2019YFA0405502 and 2019YFA0405102);Funding for the project has been provided by the National Development and Reform Commission。
Diffuse interstellar bands(DIBs)have always been a mysterious existence in astronomical research.In this work,we provide more DIB samples to slightly uncover this mystery.With the LAMOST medium-resolution survey(MRS)s...
funding agency Department of Science and Technology (DST), Government of India for providing the DST INSPIRE fellowship (IF 170830)。
In this work,we study the magnetic field morphology of selected star-forming clouds spread over the galactic latitude(b)range−10°to 10°.The polarimetric observations of clouds CB24,CB27 and CB188 are conducted to st...
Supported by the National Natural Science Foundation of China。
The composition and structure of interstellar dust are important and complex for the study of the evolution of stars and the interstellar medium(ISM).However,there is a lack of corresponding experimental data and mode...
supported by a grant from the Russian Foundation for Basic Research (18–32–00384)
The fact that infrared ring nebulae(IRRNe) are frequently associated with HⅡ regions provides us with an opportunity to study dust at the interface between ionized and neutral gas. In this paper, we analyze the assoc...