10.1126/science.276.5317.1355
Crossref journal-article
American Association for the Advancement of Science (AAAS)
Science (221)
Abstract

As stars are created by the gravitational contraction of knots in giant interstellar clouds, they shed angular momentum and magnetic and gravitational energy in an interplay of complex circumstellar structures: swirling disks, fast collimated jets, and shock waves in the surrounding cloud. Many of these structures were inferred a decade ago from ground-based telescope observations. The high resolution of the Hubble Space Telescope and other instruments has now revealed these circumstellar regions in great detail, showing features never before imagined. In the Orion Nebula alone, examples of all types of interactions between young stars and their environment can be seen simultaneously, highlighting circumstellar dynamics in sharp relief in one of astronomy’s most famous objects.

Bibliography

O’Dell, C. R., & Beckwith, S. V. W. (1997). Young Stars and Their Surroundings. Science, 276(5317), 1355–1359.

Authors 2
  1. C. Robert O’Dell (first)
  2. Steven V. W. Beckwith (additional)
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Dates
Type When
Created 23 years, 1 month ago (July 27, 2002, 5:37 a.m.)
Deposited 1 year, 7 months ago (Jan. 12, 2024, 11:03 p.m.)
Indexed 11 months, 4 weeks ago (Sept. 6, 2024, 11:45 a.m.)
Issued 28 years, 3 months ago (May 30, 1997)
Published 28 years, 3 months ago (May 30, 1997)
Published Print 28 years, 3 months ago (May 30, 1997)
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@article{O_Dell_1997, title={Young Stars and Their Surroundings}, volume={276}, ISSN={1095-9203}, url={http://dx.doi.org/10.1126/science.276.5317.1355}, DOI={10.1126/science.276.5317.1355}, number={5317}, journal={Science}, publisher={American Association for the Advancement of Science (AAAS)}, author={O’Dell, C. Robert and Beckwith, Steven V. W.}, year={1997}, month=may, pages={1355–1359} }