I've been writing an astro test based on high-mass stars/Type II SN and currently, my potential DSO list is this:BYHscioly wrote:DSO predictions:
r136a1
Eta Carinae
VY Canis Majoris
Betelguese
A few type II SNR's
Any other ideas?
Crab Pulsar
SN 1987A
Cas A
Eta Carinae
r136a1
VY Canis Majoris
M33 X-7
Cygnus X-1
Cygnus X (?)
Vela Pulsar (?)
M45 Pleiades (?)
Rosette Nebula (?)
M16 Eagle Nebula (?)
S Monocerotis (?)
V838 Monocerotis (?)
Pistol Star (?)
PSR J1748-2446ad (?)
RX J1856.5-3745 (?)
Well, the Eddington Limit is somewhat famous for being broken time and time again...Cheesy Pie wrote:Yeah that's a hypergiant in the LMC with around 286 solar masses now, and a birth mass believed to be about 360 solar masses right? Also, scientists are not sure how it got that big; above 150 solar masses, protostars should just blow themselves apart (like obese people ).
This guy seems to be doing some research with super-Eddington objects, and he argues that inhomogeneous stellar atmospheres allow the outward radiation to escape through less-dense areas, pushing less of the star's mass outwards and thus allowing objects to exist with masses above the Eddington Limit. It's worth noting as well that even the modified Eddington Limit doesn't take all potential factors into account, so maybe we shouldn't really be that surprised when the reality doesn't match up with the theory.