By Length
Full (4-12 min)
Short (1-4 min)
By Date
2024 | 2023 | 2022 | 2021
2020 | 2019 | 2018 | 2017
2016 | 2015 | 2014 | 2013
2012 | 2011 | 2010 | 2009
2008 | 2007 | 2006
By Category
Solar System
White Dwarfs
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Groups of Galaxies
Cosmology/Deep Field
Space Scoop for Kids!
Chandra Sketches
Quick Look
Visual Descriptions
How To
RSS Reader
Audio-only format podcast
Web Shortcuts
Chandra Blog
RSS Feed
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader

Tour: Astronomers See Stellar Self-Control in Action

Astronomers have found that groups of stars, or clusters, in certain environments can regulate themselves. The stars in the cluster known as RCW 36 have “self-control,” by limiting the number of stars to grow. They do this when the biggest and brightest stars expel most of the gas from the system, which depletes the cluster of the material new stars need to grow. This process could drastically slow down the birth of new stars and give better agreement with predictions for how quickly stars should be forming in clusters.

This study combines data from several telescopes including NASA's Chandra X-ray Observatory, NASA's airborne SOFIA observatory, the APEX radio telescope in Chile, and the European Space Agency’s Herschel telescope in space.

The target of the observations was RCW 36, a large cloud of gas called an HII region mainly composed of hydrogen atoms that have been ionized, which means the atoms have been stripped of their electrons. This star-forming complex is located in the Milky Way about 2,900 light-years from Earth.

RCW 36 contains a cluster of young stars and two cavities — or voids — carved out of the ionized hydrogen gas extending in opposite directions. There is also a ring of gas that wraps around the cluster in between the cavities, forming a waist around the hourglass-shaped cavities.

Astronomers see hot gas with a temperature of about two million Kelvin (or about 3.6 million degrees Fahrenheit), radiating in X-rays with Chandra. Most of the hot gas is concentrated near the center of RCW 36, close to the two hottest and most massive stars in the cluster. Much of the rest of the hot gas is outside the cavities, after having leaked through the borders of the cavities. The SOFIA and APEX data show that the ring contains cool, dense gas and is expanding at 2,000 to 4,000 miles per hour.

The SOFIA data also reveal that shells of cool gas on the perimeter of both cavities are expanding at about 10,000 miles per hour, likely being driven outward by pressure from the hot gas observed with Chandra. The hot gas, plus radiation from stars in the cluster, has also cleared even larger cavities around RCW 36, forming a structure like a nested Russian doll. Researchers also see evidence from the SOFIA data for some cool gas around the ring being ejected from RCW 36 at even higher speeds of about 30,000 miles per hour. They estimate mass equivalent to about 170 Earths are being pushed out per year.

The expansion speeds of the different structures plus the mass ejection rate show that most of the cool gas within about three light-years of the center of the HII region will be ejected from RCW 37 in one to two million years. This will clear out the raw material that stars need to form, suppressing their continued birth in the region. Astronomers call this process where stars can regulate themselves “stellar feedback.” Results such as this help us understand the role stellar feedback plays in the star formation process.

Return to Podcasts