Grid of upper atmosphere models for 1–40 M⊕ planets: application to CoRoT-7 b and HD 219134 b,c

D. Kubyshkina; L. Fossati; N. V. Erkaev; C. P. Johnstone; P. E. Cubillos; K. G. Kislyakova; H. Lammer; M. Lendl; P. Odert

doi:10.1051/0004-6361/201833737

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Volume 619 (November 2018)

A&A, 619 (2018) A151

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Table 3

X-ray and EUV luminosities adopted for each stellar mass.

M_*	L_bol	L_X1	L_X2	L_X3	L_EUV1	L_EUV2	L_EUV3
M_⊙	(10³¹ erg s⁻¹)	(10²⁴ erg s⁻¹)	(10²⁶ erg s⁻¹)	(10²⁷ erg s⁻¹)	(10²⁵ erg s⁻¹)	(10²⁷ erg s⁻¹)	(10²⁸ erg s⁻¹)
0.4	4.29	4.3	1.1	6.2	9.6	1.6	5.0
0.6	27.82	32.5	1.1	29.8	55.5	1.6	19.4
0.8	94.72	363.9	40.5	102.2	438.8	34.9	55.8
1.0	266.41	363.9	40.5	286.8	438.8	34.9	135.7
1.3	942.41	942.4	73.2	1011.4	995.1	58.5	402.2

Notes. The subscripts “1”, “2”, and “3” indicate cases of inactive, moderately active, and active stars, respectively.

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