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Stars determine their own masses | PressReleasePoint - Vimarsana News

Stars determine their own masses | PressReleasePoint

In theory, masses of stars should vary wildly, yet mass distribution is nearly universal New simulations show that star formation is a self-regulatory process In an effort to oppose gravity, stellar feedback pushes stellar masses toward the same mass distribution.

New Study Sheds Light on Why Stellar Populations Are So Similar in Milky Way - Vimarsana News

New Study Sheds Light on Why Stellar Populations Are So Similar in Milky Way

Cambridge, MA – Scientists have uncovered what sets the masses of stars, a mystery that has captivated astrophysicists for decades. Their answer? Stars, themselves.

The Weekend Ahead: happenings on campus, in Evanston July 29-31 - Vimarsana News

The Weekend Ahead: happenings on campus, in Evanston July 29-31

The Weekend Ahead is back for the summer. Over the next few months, we’ll highlight events both on campus and in Evanston. Read on to find your weekend plans. Northwestern events “Dance Nation”  Virginia Wadsworth Wirtz Center for the Performing Arts Friday and Saturday at 7:30 p.m.; Saturday and Sunday at 2 p.m. $6 in...

Science News | Study: Blinking Gamma Ray Bursts Are Explained by Falling Stardust and Unsteady Jets - Vimarsana News

Science News | Study: Blinking Gamma Ray Bursts Are Explained by Falling Stardust and Unsteady Jets

Get latest articles and stories on Science at LatestLY. Astrophysicists have developed the first 3D simulation of the entire evolution of a jet from its birth by a rotating black hole to its emission far from the collapsing star. Science News | Study: Blinking Gamma Ray Bursts Are Explained by Falling Stardust and Unsteady Jets.

Study: Blinking gamma ray bursts are explained by falling stardust and unsteady jets - Vimarsana News

Study: Blinking gamma ray bursts are explained by falling stardust and unsteady jets

Astrophysicists have developed the first 3D simulation of the entire evolution of a jet from its birth by a rotating black hole to its emission far from the collapsing star.