May 9, 2014
No Writer Credit
Over ninety percent of the stars in our galaxy were born in stellar nurseries, clusters of stars nestled deep within clouds of dust and molecular gas. These young natal environments are key targets for astronomers who study star formation because they retain imprints of the initial conditions that produced the stars and the dynamical environments under which they evolved. Clusters with massive stars (stars more than a few solar masses in size) are of particular interest since both the formation of massive stars and their impact on other cluster members are poorly understood, for several fundamental reasons. Massive stars begin hydrogen burning while they are still growing and hence quickly develop strong winds and ultraviolet radiation that inhibit their further growth while at the same time disrupting the nursery with shock waves and ionizing light. Moreover, because massive stars evolve quickly they do not linger in any particular stage of development long enough for easy study, and they remain obscured by the not-yet-disbursed natal dust. None of these issues applies to the formation of lower mass stars.
A Spitzer three-color infrared image of the massive star-forming cluster in the W5-East molecular cloud. CfA astronomers have used the infrared images to survey the populations of embedded young stars in this and four other regions. The contours show the extent of ionizing radiation from embedded stars; white arrows show radiation from external, hot stars. The scale marker indicates a length of 6.58 light-years.
CfA astronomers Luis Chavarria, Joe Hora, Gus Muench, and Giovanni Fazio and two colleagues undertook a study of massive stellar clusters with the Spitzer Space Telescope, whose infrared camera can peer inside dusty regions. They chose five massive clusters relatively nearby (about six thousand light-years) and performed a detailed census of their populations using the infrared colors of the individual stars to characterize the clusters’ sizes and stages of development.
The astronomers report finding 3021 young stars in their set of five clusters, a large enough sample to draw significant conclusions. The youngest group of these stars, a subset of 539, are found in regions where the cloud material is densest, supporting the general picture of cluster formation. The scientists also find that massive young stars form preferentially in filamentary (rather than spherical) structures that subsequently fragment, probably due to turbulence effects.
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The Center for Astrophysics combines the resources and research facilities of the Harvard College Observatory and the Smithsonian Astrophysical Observatory under a single director to pursue studies of those basic physical processes that determine the nature and evolution of the universe. The Smithsonian Astrophysical Observatory (SAO) is a bureau of the Smithsonian Institution, founded in 1890. The Harvard College Observatory (HCO), founded in 1839, is a research institution of the Faculty of Arts and Sciences, Harvard University, and provides facilities and substantial other support for teaching activities of the Department of Astronomy. The long relationship between the two organizations, which began when the SAO moved its headquarters to Cambridge in 1955, was formalized by the establishment of a joint center in 1973. The CfA’s history of accomplishments in astronomy and astrophysics is reflected in a wide range of awards and prizes received by individual CfA scientists.
Today, some 300 Smithsonian and Harvard scientists cooperate in broad programs of astrophysical research supported by Federal appropriations and University funds as well as contracts and grants from government agencies. These scientific investigations, touching on almost all major topics in astronomy, are organized into the following divisions, scientific departments and service groups.
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