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Cone Nebula (NGC 2264): Star-Forming Pillar of Gas and Dust

Cone Nebula (NGC 2264): Star-Forming Pillar of Gas and Dust

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Credit: NASA, H. Ford (JHU), G. Illingworth (UCSC/LO), M.Clampin (STScI), G. Hartig (STScI), the ACS Science Team, and ESA

The ACS Science Team: H. Ford, G. Illingworth, M. Clampin, G. Hartig, T. Allen, K. Anderson, F. Bartko, N. Benitez, J. Blakeslee, R. Bouwens, T. Broadhurst, R. Brown, C. Burrows, D. Campbell, E. Cheng, N. Cross, P. Feldman, M. Franx, D. Golimowski, C. Gronwall, R. Kimble, J. Krist, M. Lesser, D. Magee, A. Martel, W. J. McCann, G. Meurer, G. Miley, M. Postman, P. Rosati, M. Sirianni, W. Sparks, P. Sullivan, H. Tran, Z. Tsvetanov, R. White, and R. Woodruff.

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Edifice of Gas and Dust in the Cone NebulaDense Gas and Dust Beyond the Outer Layers of the Cone NebulaThe Cone Nebula (NGC 2264)Hubble Snaps Selecting this will take you out of this index and relocate you to a Gallery Search Results page.