arXiv Open Access 2023

Planetary line-to-accretion luminosity scaling relations: Extrapolating to higher-order hydrogen lines

Gabriel-Dominique Marleau Yuhiko Aoyama
Lihat Sumber

Abstrak

Aoyama et al. (2021, ApJL) provided scaling relations between hydrogen-line luminosities and the accretion luminosity for planetary-mass objects. These fits should be an improvement over blind extrapolations of stellar relations. The fits go up only to the n = 8 electron energy level, but higher-n Balmer lines have been observed in the near-UV at Delorme 1 (AB)b with UVES (Ringqvist et al. 2023). We extend the scaling relations to higher-n levels for the Balmer and other series by fitting the fit coefficients (a, b) themselves and extrapolating them. Within the assumption of an accretion shock as the source of line emission, these fits should be robust for accreting planetary-mass objects.

Topik & Kata Kunci

Penulis (2)

G

Gabriel-Dominique Marleau

Y

Yuhiko Aoyama

Format Sitasi

Marleau, G., Aoyama, Y. (2023). Planetary line-to-accretion luminosity scaling relations: Extrapolating to higher-order hydrogen lines. https://arxiv.org/abs/2303.00011

Akses Cepat

Lihat di Sumber
Informasi Jurnal
Tahun Terbit
2023
Bahasa
en
Sumber Database
arXiv
Akses
Open Access ✓