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The Interstellar Medium (ISM): The Birth of Stars

Discover the interstellar medium, where gas and dust form stars in nebulae. Learn about radio telescopes, molecules in space, and supernovae effects on star birth in our Galaxy.

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The Interstellar Medium (ISM): The Birth of Stars

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  1. The Interstellar Medium (ISM):The Birth of Stars

  2. Interstellar gas and dust pervade the Galaxy • Interstellar gas and dust, which make up the interstellar medium, are concentrated in the disk of the Galaxy • Clouds within the interstellar medium are called nebulae • Dark nebulae are so dense that they are opaque • They appear as dark blots against a background of distant stars • Emission nebulae, or H II regions, are glowing, ionized clouds of gas • Emission nebulae are powered by ultraviolet light that they absorb from nearby hot stars • Reflection nebulae are produced when starlight is reflected from dust grains in the interstellar medium, producing a characteristic bluish glow

  3. A radio telescope uses a large concave dish to reflect radio waves to a focus • Radio telescopes use large reflecting antennas or dishes to focus radio waves • Very large dishes provide reasonably sharp radio images

  4. Higher resolution is achieved with interferometry techniques that link smaller dishes together

  5. The spin-flip transition in hydrogen emits 21-cm radio waves

  6. Molecules in Space • 130 known molecules • Some molecules contain 13 atoms • http://www.ph1.uni-koeln.de/vorhersagen • A 9 atom molecule … C2H5OH …ethanol

  7. Star birth can begin in giant molecular clouds The spiral arms of our Galaxy are laced with giant molecular clouds, immense nebulae so cold that their constituent atoms can form into molecules

  8. Star-forming regions appear when a giant molecular cloud is compressed • This can be caused by the cloud’s passage through one of the spiral arms of our Galaxy, by a supernova explosion, or by other mechanisms

  9. Protostars form in cold, dark nebulae • Star formation begins in dense, cold nebulae, where gravitational attraction causes a clump of material to condense into a protostar • As a protostar grows by the gravitational accretion of gases, Kelvin-Helmholtz contraction causes it to heat and begin glowing

  10. A circumstellar accretion disk provides material that a young star ejects as jets

  11. Young star clusters give insight into starformation and evolution • Newborn stars may form an open or galactic cluster • Stars are held together in such a cluster by gravity • Occasionally a star moving more rapidly than average will escape, or “evaporate,” from such a cluster • A stellar association is a group of newborn stars that are moving apart so rapidly that their gravitational attraction for one another cannot pull them into orbit about one another

  12. Supernovae compress the interstellar mediumand can trigger star birth

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