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Date Published: 30/09/2024
Online Published: 30/09/2024
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DOI: https://doi.org/10.54607/hcmue.js.21.9.4459(2024)
Issue
Vol. 21 No. 9 (2024)
Section
Articles
How to Cite
Phan , B. N. (2024). DENIS-P J1901391-370017: IS A YOUNG VERY LOW-MASS STAR OR A LOW-MASS BROWN DWARF IN CORONA-AUSTRALIS?. HCMUE Journal of Science, 21(9), 1576. https://doi.org/10.54607/hcmue.js.21.9.4459(2024)

DENIS-P J1901391-370017: IS A YOUNG VERY LOW-MASS STAR OR A LOW-MASS BROWN DWARF IN CORONA-AUSTRALIS?

Bảo Ngọc Phan

Main Article Content

Abstract

DENIS-P J1901391-370017 has been identified as a low-mass brown dwarf in the Corona-Australis cloud. This paper presents our mass estimate of this brown dwarf. The dereddened spectral energy distribution of the source indicates that DENIS-P J1901391-370017 is a very low-mass star, not a low-mass brown dwarf, as previously reported. We also reconfirm that DENIS-P J1901391-370017 is diskless, as previously mentioned in the literature.

 

Keywords

brown dwarfs, circumstellar matter, photometry, spectroscopy

Article Details

References

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