Extreme star cluster bursts into life in new Hubble image

Oct 02, 2007
Nebula NGC 3603
This Hubble image shows the gigantic nebula NGC 3603 located in the Carina spiral arm of the Milky Way, about 20,000 light-years from the Solar System. NGC 3603 hosts one of the most prominent, massive, young clusters in the Milky Way. Hubble has been observing this prime location for star formation studies. The images show a young star cluster surrounded by a vast region of dust and gas. Most of the bright stars in the image are hot, blue stars. They produce ultraviolet radiation and violent winds that have formed an enormous cavity in the gas and dust surrounding the cluster. Credit: NASA/ ESA/ STScI/Aura (The hubble heritage team)

The gigantic nebula NGC 3603 hosts one of the most prominent, massive, young clusters in the Milky Way. Hubble has been observing this prime location for star formation studies.

NGC 3603 is located in the Carina spiral arm of the Milky Way, about 20 000 light-years from the Solar System.

Images from the NASA/ESA Hubble Space Telescope show a young star cluster surrounded by a vast region of dust and gas. Most of the bright stars in the image are hot, blue stars. They produce ultraviolet radiation and violent winds that have formed an enormous cavity in the gas and dust surrounding the cluster.

The image shows many stars with differing masses but similar ages inside the young cluster. Stars of different masses evolve at a different pace, so this makes it possible to study several types of stars at varying stages in their lives, in detail. Astronomers can compare clusters of different ages with one another and determine which properties (such as temperature and brightness) change as the stars get older.

Dr Jesús Maíz Apellániz from Instituto de Astrofísica de Andalucía, Spain, is leading the Hubble investigation. According to him, the cluster appears to gather the most massive stars at its core. His team has discovered that the distribution of different types of stars at the centre of this dense cluster is similar to that of other young clusters in the Milky Way.

Apellániz's team has also found that the three brightest stars in the centre appear to be more massive than theoretical limits allow. In fact, these ‘heavyweights’ may actually consist of two or perhaps more individual massive stars whose light has blended together. Even with Hubble’s resolution, it is not possible to separate the individual stars in each of the three systems.

This finding agrees with a recent discovery by Dr. Anthony Moffat from the Université de Montréal, Canada. He used ESO’s Very Large Telescope (VLT) and Hubble’s Near Infrared Camera and Multi-Object Spectrograph (NICMOS) to measure the movements of the individual stars in two of the three systems. Dr. Moffat measured the largest star’s mass to be roughly 115 times that of the Sun - which is within acceptable limits for conventional theory.

The swirling nebula of NGC 3603 contains around 400 000 solar masses of gas. Lurking within this vast cloud are a few Bok globules, named after Bart Bok who first observed them in the 1940s.

Bok globules are dark clouds of dense dust and gas with masses of about ten to fifty times that of the Sun. They resemble insect cocoons and are in the process of collapsing under their own weight, forming new stars. Bok globules appear to be some of the coldest objects in the Universe.

NGC 3603 was first discovered by Sir John Herschel in 1834. It is known to harbour a blue supergiant star called Sher 25, believed to be on the verge of exploding as a supernova. It is often known as the Milky Way counterpart of the predecessor of the now-famous supernova SN 1987A in the Large Magellanic Cloud.

Source: European Space Agency

Explore further: Fermi finds a 'transformer' pulsar

add to favorites email to friend print save as pdf

Related Stories

'A drop of ink on the luminous sky'

Feb 13, 2013

This part of the constellation of Sagittarius (The Archer) is one of the richest star fields in the whole sky—the Large Sagittarius Star Cloud. The huge number of stars that light up this region dramatically ...

An angry bird in the sky

Sep 21, 2011

(PhysOrg.com) -- A new image from the Wide Field Imager on the MPG/ESO 2.2-metre telescope reveals the Lambda Centauri Nebula, a cloud of glowing hydrogen and newborn stars in the constellation of Centaurus ...

Recommended for you

Fermi finds a 'transformer' pulsar

5 hours ago

(Phys.org) —In late June 2013, an exceptional binary containing a rapidly spinning neutron star underwent a dramatic change in behavior never before observed. The pulsar's radio beacon vanished, while at ...

Transiting exoplanet with longest known year

Jul 21, 2014

Astronomers have discovered a transiting exoplanet with the longest known year. Kepler-421b circles its star once every 704 days. In comparison, Mars orbits our Sun once every 780 days. Most of the 1,800-plus ...

User comments : 1

Adjust slider to filter visible comments by rank

Display comments: newest first

holoman
3 / 5 (1) Oct 02, 2007
Wow ! these are some great images from Hubble.

http://hubblesite...scenter/
http://heritage.s...dex.html