SISSI: Supernovae in a stratified, shearing interstellar medium - II. Star formation near the Sun is quenched by expansion of the Local Bubble

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Table B.1

Properties of the Local Bubble

Property	This work	Z+22	O+24	Unit
Effective Radius	212.3 ± 1.0_stat	165 ± 6	170^a	pc
Mass	6.2 ± 0.7_sys ± 0.07_stat	$14_{- 6.2}^{+ 6.5}$ $Mathematical equation: $14_{-6.2}^{+6.5}$$	6.0 ± 0.7^b	10⁵ M_⊙
Hydrogen number density	0.50 ± 0.06_sys ± 0.006_stat	$2 . 71_{- 1.02}^{+ 1.57}$ $Mathematical equation: $2.71_{-1.02}^{+1.57}$$	0.61^c	cm⁻³
Momentum	(3.0 ± 1.7_sys ± 0.05_stat)^d ×(Myr/t_age)	$1 . 0_{- 0.4}^{+ 0.4}$ $Mathematical equation: $1.0_{-0.4}^{+0.4}$$	–	10⁷ M_⊙ km s⁻¹
Minor-to-major-ratio	0.469 ± 0.007	–	–	–
Semi-major-to-major-ratio	0.562 ± 0.011	–	–	–
Pitch angle (major axis)	−19.0 ± 1.0	–	–	。
Polar direction (major axis)	0.665 ± 0.011	–	–	–
Pitch angle (minor axis)	–66.1 ± 2.7	–	–	。
Polar direction (minor axis)	0.607 ± 0.022	–	–	–

^(a) Median peak distance ^(b) Mass enclosed within shell ^(c) Median peak density ^(d) Bias corrected (see Appendix C.1)

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