Hubble image archive

Westerlund 2: Detail 3

The pillars in the star-forming region surrounding Westerlund 2, composed of dense gas, are a few light-years tall and point to the central cluster. They are thought to be incubators for new stars. Besides sculpting the gaseous terrain, intense radiation from the most brilliant o...

Date
Jan 1, 2015
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-2015-12-3520-image
By

The pillars in the star-forming region surrounding Westerlund 2, composed of dense gas, are a few light-years tall and point to the central cluster. They are thought to be incubators for new stars. Besides sculpting the gaseous terrain, intense radiation from the most brilliant of the cluster stars is creating a successive generation of baby stars. The bluish haze is an indicator of oxygen gas in the nebula.

Credits

NASA, ESA, the Hubble Heritage Team (STScI/AURA), A. Nota (ESA/STScI), and the Westerlund 2 Science Team

Image Details

About The Object
Object NameWesterlund 2, Gum 29
Object DescriptionCluster and Starforming Region
R.A. Position10h 23m 58.1s
Dec. Position-57° 45' 48.96"
ConstellationCarina
Distance20,000 light-years (6,130 parsecs)
About The Data
Data DescriptionData of Westerlund 2 were obtained from the HST proposals : A. Nota (ESA/STScI), E. Sabbi and C. Christian (STScI), E. Grebel and P. Zeidler (Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg), M. Tosi (INAF, Osservatorio Astronomico di Bologna), A. Bonanos (National Observatory of Athens, Astronomical Institute), and S. de Mink (University of Amsterdam); and : Z. Levay, M. Mutchler, J. Mack, L. Frattare, S. Meyett, M. Livio, and C. Christian (STScI/AURA), K. Noll (NASA/GSFC), A. Nota (STScI/ESA), and E. Sabbi (STScI).
InstrumentHST>ACS/WFC and HST>WFC3/IR
Exposure DatesSeptember 2013 - November 2014, Total Exposure Time: 23,074 seconds
FiltersACS/WFC: F555W (V) and F814W (I) WFC3/IR: F125W (J)
About The Image
Color InfoThese images are composites of separate exposures acquired by the ACS and the WFC3 instruments on the Hubble Space Telescope. Several filters were used to sample broad and narrow wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue: F555W (V) Green: F555W (V) and F814W (I) Red: F814W (I)

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