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Introduction Press Release Visuals More Info

image
NASA/CXC/JPL-Caltech/PSU/CfA

Trigger-Happy Cloud

This composite image, combining data from NASA's Chandra X-ray Observatory and Spitzer Space Telescope shows the star-forming cloud Cepheus B, located in our Milky Way galaxy about 2,400 light years from Earth. A molecular cloud is a region containing cool interstellar gas and dust left over from the formation of the galaxy and mostly
contains molecular hydrogen. The Spitzer data, in red, green and blue shows the molecular cloud (in the bottom part of the image) plus young stars in and around Cepheus B, and the Chandra data in violet shows the young stars in the field.

The Chandra observations allowed the astronomers to pick out young stars within and near Cepheus B, identified by their strong X-ray emission. The Spitzer data showed whether the young stars have a so-called "protoplanetary" disk around them. Such disks only exist in very young systems where planets are still forming, so their presence is an
indication of the age of a star system.

These data provide an excellent opportunity to test a model for how stars form. The new study suggests that star formation in Cepheus B is mainly triggered by radiation from one bright, massive star (HD 217086) outside the molecular cloud. According to the particular model of triggered star formation that was tested -- called the radiation-
driven implosion model -- radiation from this massive star drives a compression wave into the cloud triggering star formation in the interior, while evaporating the cloud's outer layers.

Different types of triggered star formation have been observed in other environments. For example, the formation of our solar system was thought to have been triggered by a supernova explosion. In the star-forming region W5, a "collect-and-collapse" mechanism is thought to apply, where shock fronts generated by massive stars sweep up material
as they progress outwards. Eventually the accumulated gas becomes dense enough to collapse and form hundreds of stars. The radiation-driven implosion model mechanism is also thought to be responsible for the formation of dozens of stars in W5. The main cause of star formation that does not involve triggering is where a cloud of gas cools, gravity gets the upper hand, and the cloud falls in on itself.

To download, choose your preferred resolution and file format below. "High-Resolution" files will always be the highest resolution and widest crop available, intended for print. Other resolutions are provided for convenient on-screen viewing.

Screen-Resolution (600x750) : JPEG (176 KB)
Medium-Resolution (1200x1500) : JPEG (256 KB)
High-Resolution (2400x3000) : JPEG (2.1 MB) | Mac TIFF (5.2 MB)

About the Object (1)
Object name:Cepheus B
Object type:Star Forming Region, Nebula
Position (J2000):RA: 22h 56m 46.99s  Dec: 62° 40' 0.00"
Distance:2,365 Ligh Years
Constellation:Cepheus
About the Data
Spitzer Data
Image Credit:NASA/CXC/JPL-Caltech/PSU/CfA
Instrument:IRAC
Release Date:2009/08/12

Additional Info
Press Release: Space Telescopes Find Trigger-Happy Star Formation

INDIVIDUAL IMAGES

Trigger-Happy Cloud - Without Labels

Screen-Resolution (573x750): JPEG
High-Resolution (2749x3600): JPEG | Mac TIFF
Credit: NASA/CXC/JPL-Caltech/PSU/CfA

Introduction Press Release Visuals More Info



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