From 40a9500a6db298f5a11f964496ab7ddd1a66bc37 Mon Sep 17 00:00:00 2001 From: Jeff Riley Date: Fri, 29 Nov 2024 08:42:08 +1100 Subject: [PATCH] fixed bulleted list on whats-new page --- online-docs/pages/whats-new.rst | 6 ++---- 1 file changed, 2 insertions(+), 4 deletions(-) diff --git a/online-docs/pages/whats-new.rst b/online-docs/pages/whats-new.rst index b0ad3b284..7e98516bd 100644 --- a/online-docs/pages/whats-new.rst +++ b/online-docs/pages/whats-new.rst @@ -28,13 +28,11 @@ Improved the treatment of stellar rotation (with further corrections in 03.08.01 * Assume rigid body rotation * Keep the angular moment of a star constant when there is no mass loss -* When a star with radius r and angular frequency omega loses mass dm through winds or mass transfer, it loses angular momentum dL = -(2/3) dm r^2 omega +* When a star with radius r and angular frequency omega loses mass dm through winds or mass transfer, it loses angular momentum dL = (2/3) dm r^2 omega * (However, angular momentum never drops below zero) * When a star loses its envelope, the remaining core is assumed to rotate with the same rotation rate as the preceding star * When a star of mass m and radius r gains mass dm through accretion, it gain angular momentum dL = dm \sqrt{G m r} -* If initial binary rotation is fast enough for a star to be CHE, it is set to that rotation frequency without regard for the tidal -prescription; CHE stars remain tidally locked if the tidal prescription is NONE +* If initial binary rotation is fast enough for a star to be CHE, it is set to that rotation frequency without regard for the tidal prescription; CHE stars remain tidally locked if the tidal prescription is NONE **03.07.01 Oct 23, 2024**