{"title":"Gaia EDR3 Data For Three Young Stellar Objects","authors":"K. Gigoyan, N. Azatyan, K. Gigoyan","doi":"10.52526/25792776-22.69.1-77","DOIUrl":null,"url":null,"abstract":"We present Gaia Early Data Release 3 (Gaia EDR3) high accurate astrometric and photometric data\nand also Catalina Sky Survey (CSS ) phase-dependent light curves for three Young Stellar Objects (YSO).\nThey are LRL 245, 2MASS J04300424+3533238, and CVSO 592. These tree YSOs are presented as periodic variables in the Catalina Surveys Data Release-1 (CSDR1) data base.\nCSS phase-dependent curve of LRL 245 shows periodicity with period P=234.66 days and amplitude\n∆m≈4.0 mag. For this object high-resolution spectra in H-band (from 1.51 to 1.69 µm) was obtained by\nthe APOGEE instrument. LAMOST telescope moderate-resolution CCD spectra is available for object\n2MASS J04300424+3522238 only. The spectra shows clear features of M dwarfs.","PeriodicalId":412578,"journal":{"name":"Communications of the Byurakan Astrophysical Observatory","volume":"6 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-09-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Communications of the Byurakan Astrophysical Observatory","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.52526/25792776-22.69.1-77","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
We present Gaia Early Data Release 3 (Gaia EDR3) high accurate astrometric and photometric data
and also Catalina Sky Survey (CSS ) phase-dependent light curves for three Young Stellar Objects (YSO).
They are LRL 245, 2MASS J04300424+3533238, and CVSO 592. These tree YSOs are presented as periodic variables in the Catalina Surveys Data Release-1 (CSDR1) data base.
CSS phase-dependent curve of LRL 245 shows periodicity with period P=234.66 days and amplitude
∆m≈4.0 mag. For this object high-resolution spectra in H-band (from 1.51 to 1.69 µm) was obtained by
the APOGEE instrument. LAMOST telescope moderate-resolution CCD spectra is available for object
2MASS J04300424+3522238 only. The spectra shows clear features of M dwarfs.