PENELLOPE - VII. Revisiting empirical relations to measure accretion luminosity

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Volume 704 (December 2025)

A&A, 704 (2025) A42

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Table 1

Stellar extinction and accretion luminosities.


Region	Source name	$A_{V}^{W}$ $\[A_{V}^{W}\]$ mag	log $L_{acc}^{l i n e s - W}$ $\[L_{\text {acc }}^{lines-W}\]$ L_⊙	$A_{V}^{n o t W}$ $\[A_{V}^{not W}\]$ mag	log $L_{acc}^{l i n e s - n o t W}$ $\[L_{\text {acc }}^{lines-not W}\]$ L_⊙	$A_{V}^{d i f f}$ $\[A_{V}^{diff}\]$ mag	log $L_{a c c}^{l i n e s - d i f f}$ $\[L_{\mathrm{acc}}^{lines-diff}\]$ L_⊙	log $L_{acc}^{l i n e s, T W}$ $\[L_{\text {acc }}^{lines, T W}\]$ L_⊙	ΔT day
OB1	CVSO58	${0.7}_{- 0.6}^{+ 0.8}$ $\[0.7_{-0.6}^{+0.8}\]$	−1.45 ± 0.15	${0.9}_{- 0.8}^{+ 1.1}$ $\[0.9_{-0.8}^{+1.1}\]$	−1.45 ± 0.18	${1.0}_{- 0.2}^{+ 0.2}$ $\[1.0_{-0.2}^{+0.2}\]$	−1.30 ± 0.18	−0.65 ± 0.23	0.26
OB1	CVSO90	${2.4}_{- 2.2}^{+ 2.6}$ $\[2.4_{-2.2}^{+2.6}\]$	0.08 ± 0.37	${1.1}_{- 0.9}^{+ 1.3}$ $\[1.1_{-0.9}^{+1.3}\]$	0.08 ± 0.17	${1.1}_{- 0.2}^{+ 0.2}$ $\[1.1_{-0.2}^{+0.2}\]$	−0.55 ± 0.17	−0.27 ± 0.27	1.57
OB1	CVSO104	${1.4}_{- 1.3}^{+ 1.6}$ $\[1.4_{-1.3}^{+1.6}\]$	−0.89 ± 0.36	${0.2}_{- 0.0}^{+ 0.4}$ $\[0.2_{-0.0}^{+0.4}\]$	−0.89 ± 0.21	${0.2}_{- 0.2}^{+ 0.2}$ $\[0.2_{-0.2}^{+0.2}\]$	−1.38 ± 0.21	−0.75 ± 0.26	0.10
...	...	...	...	...	...	...	...	...	...
...	...	...	...	...	...	...	...	...	...

Notes. A_V and L_acc are computed using the three minimizing methodologies (see Sect. 3.6) and the HST modelling (see Sect. 3.3). The last column show the difference in time between XS and HST observations. Only the first entries are shown; a complete version of this table is available at the CDS.

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