Skip to main content

A Superluminous Supernova from a Massive Progenitor Star

Submitted by mjuliano-adm on
Stars greater than about eight solar-masses end their lives spectacularly as supernovae. These single-star supernovae are called core collapse supernovae because their dense cores, compos...

Advancement

Submitted by tyler.jump on
A core focus of SAO's work as a Smithsonian research unit is to serve the American public through a commitment to cutting-edge scientific research and provide free and equitable access to...

The Youngest Stellar Embryos in Massive Clouds

Submitted by mjuliano-adm on
Stars form as gravity contracts the gas and dust in an interstellar cloud until cores develop that are dense enough to coalesce into stars. A dense core in the earliest phase of this proc...

The Diversity and Variability of Star Formation

Submitted by mjuliano-adm on
Galaxies in the observable universe show a remarkable diversity in their structure and properties, mostly because of the many different pathways for their stars to form and evolve. The gr...

Dust Grains from Supernovae

Submitted by mjuliano-adm on
Dust grains in the interstellar medium are responsible for the dramatic shapes darkening the faces of bright nebulae, the Horsehead Nebula for example. The grains absorb ultraviolet and o...
Subscribe to