Understanding post-red giant branch binaries through stable mass transfer

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Volume 703 (November 2025)

A&A, 703 (2025) A294

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Table C.3.

SED fitting results of the post-AGB and post-RGB binary candidate samples in the LMC and SMC.

Object	Host	T_eff/K	E(B − V)	L/L_⊙	L_IR/L_* (%)	Reference
J045745.46-683724.1	LMC	7131	0.0 $_{- 0.00}^{+ 0.28}$ $_{-0.00}^{+0.28}$	81 $_{- 1}^{+ 115}$ $_{-1}^{+115}$	67	(2)
J054144.88-712351.7	LMC	4946	0.0 $_{- 0.00}^{+ 0.34}$ $_{-0.00}^{+0.34}$	88 $_{- 0}^{+ 72}$ $_{-0}^{+72}$	38	(2)
J053811.63-680824.9	LMC	5421	0.11 $_{- 0.11}^{+ 0.13}$ $_{-0.11}^{+0.13}$	94 $_{- 16}^{+ 28}$ $_{-16}^{+28}$	27	(2)
J053030.78-701805.5	LMC	4754	0.03 $_{- 0.03}^{+ 0.19}$ $_{-0.03}^{+0.19}$	99 $_{- 4}^{+ 34}$ $_{-4}^{+34}$	85	(2)
J051412.13-702026.0	LMC	7133	0.05 $_{- 0.05}^{+ 0.27}$ $_{-0.05}^{+0.27}$	112 $_{- 14}^{+ 149}$ $_{-14}^{+149}$	92	(2)
J045836.92-701120.1	LMC	8250	0.14 $_{- 0.14}^{+ 0.24}$ $_{-0.14}^{+0.24}$	115 $_{- 39}^{+ 177}$ $_{-39}^{+177}$	239	(2)
J051751.41-713507.3	LMC	8225	0.28 $_{- 0.21}^{+ 0.17}$ $_{-0.21}^{+0.17}$	121 $_{- 56}^{+ 102}$ $_{-56}^{+102}$	72	(2)
J045736.84-705127.2	LMC	10480	0.2 $_{- 0.07}^{+ 0.04}$ $_{-0.07}^{+0.04}$	131 $_{- 35}^{+ 30}$ $_{-35}^{+30}$	28	(2)
J052107.90-714104.4	LMC	10500	0.13 $_{- 0.13}^{+ 0.10}$ $_{-0.13}^{+0.10}$	131 $_{- 54}^{+ 86}$ $_{-54}^{+86}$	81	(2)
(...)	(...)	(...)	(...)	(...)	(...)	(...)

Notes. The table lists the following information for each object: its identification, host Magellanic Cloud, effective temperature T_eff, reddening E(B − V), luminosity L, IR-to-stellar luminosity ratio L_IR/L_*, and the reference to the paper from which the object was taken. The effective temperatures have a formal error of ±250 K. The distances used to determine the luminosities were 50 kpc for the LMC (Walker 2012; Pietrzyński et al. 2013) and 62 kpc for the SMC (Graczyk et al. 2013). The whole table is available at CDS.

References. (1) van Aarle et al. (2011); (2) Kamath et al. (2015); (3) Manick et al. (2018); (4) Kamath et al. (2014).

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