MK-like spectral classification for hot subdwarf stars with LAMOST spectra
Fuente:
arXiv
Salvato in:
| Autori principali: | , |
|---|---|
| Natura: | Preprint |
| Pubblicazione: |
2024
|
| Soggetti: | |
| Accesso online: | |
| Tags: |
Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
|
| _version_ | 1866911965611294720 |
|---|---|
| author | Zou, Xuan Lei, Zhenxin |
| author_facet | Zou, Xuan Lei, Zhenxin |
| contents | An MK-like spectral classification has been conducted for 1224 hot subdwarf stars with LAMOST DR9 low-resolution spectra. The whole sample was divided into four categories according to the spectral line characteristics: He-normal, He-weak, He-strong C and He-strong. Each selected spectrum was assigned a spectral class, a luminosity class and an helium class by comparing the line depth and width with standard spectra selected in LAMOST. Relationships between atmospheric parameters and spectral classification were also presented. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_17062 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | MK-like spectral classification for hot subdwarf stars with LAMOST spectra Zou, Xuan Lei, Zhenxin Solar and Stellar Astrophysics An MK-like spectral classification has been conducted for 1224 hot subdwarf stars with LAMOST DR9 low-resolution spectra. The whole sample was divided into four categories according to the spectral line characteristics: He-normal, He-weak, He-strong C and He-strong. Each selected spectrum was assigned a spectral class, a luminosity class and an helium class by comparing the line depth and width with standard spectra selected in LAMOST. Relationships between atmospheric parameters and spectral classification were also presented. |
| title | MK-like spectral classification for hot subdwarf stars with LAMOST spectra |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2407.17062 |