The Universe has countless stars, which come in different masses. The most common ones are the low-mass stars, including our Sun. Massive stars refer to those whose mass is more than eight times the mass of the Sun. The life of low-mass stars is quite long. For instance, our Sun can live for 10 billion years. However, massive stars can only live up to tens of millions of years.

Some of these massive stars will have a splendid death. They can explode as core-collapse supernovae, which can outshine their entire galaxy. More than 2000 years ago (in the Han Dynasty), ancient Chinese astronomers kept records of the earliest supernovae observed with naked eyes by humankind.

Supernova events are rare in our galaxy due to the low star formation rate of the Milky Way. That is to say, there are not many baby stars born every year.

However, in starburst galaxies, the star formation rate can be boosted by a factor of 10 or 100! Accordingly, starburst galaxies can put on a "fireworks show" of supernovae when massive stars die. Arp 299 is a pair of colliding galaxies where numerous supernovae have exploded. In fact, it puts on at least a few "fireworks shows" of supernovae per decade.

Supernovae release not only a massive amount of photons (energy) but also a large number of elements (matter), such as oxygen, neon, magnesium, and iron. The relative amount of different elements is quite sensitive to the population of massive stars that die as core-collapse supernovae.

Using ESA's XMM-Newton space observatory, an international group of astronomers measured the chemical composition of the X-ray emitting "confetti" in Arp 299.

It is often assumed that massive stars from 10 to 40 times the mass of the Sun can explode successfully as core-collapse supernovae. However, the observed chemical composition in Arp 299 does not match the existing theoretical models unless we remove supernovae from massive stars heavier than 23 to 27 times the mass of the Sun. This is in accordance with the fact that astronomers have not clearly observed supernovae from stars heavier than 18 times the mass of the Sun.

What happens to those massive stars, then? They might end their life as black holes with no matter escaping from it or less energetic supernovae that release a little matter. The research team also points out that it is also possible that current theoretical predictions of the elements released through core-collapse supernovae are underestimated.

Research Report: "Elemental Abundances of the Hot Atmosphere of Luminous Infrared Galaxy Arp 299"

Related Links
Hiroshima University
Stellar Chemistry, The Universe And All Within It

Thanks for being there; We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain. With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords. Our news coverage takes time and effort to publish 365 days a year. If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.
SpaceDaily Monthly Supporter $5+ Billed Monthly		SpaceDaily Contributor $5 Billed Once credit card or paypal

What can a young star teach us about the birth of our solar system
Boston MA (SPX) Sep 02, 2021
The familiar star at the center of our solar system has had billions of years to mature and ultimately provide life-giving energy to us here on Earth. But a very long time ago, our sun was just a growing baby star. What did the sun look like when it was so young? That's long been a mystery that, if solved, could teach us about the formation of our solar system-so-named because sol is the Latin word for sun-and other stellar systems made up of planets and cosmic objects orbiting stars. "We've detec ... read more

Read more from original source...