Abstract
It is now known that molecular clouds are the sites of star formation in the Galaxy. Forty years ago, however, it was not clear that molecules were even an important constituent of the Galaxy. In 1955, Townes [1] presented a paper at IAU Symposium 4 in which he listed a number of molecules that might have radio transitions. Thirteen years after this conference, Townes and his collaborators [2] discovered the first polyatomic molecule in interstellar space, NH3. Now, with more powerful radio telescopes, ammonia is used to trace regions in which low mass stars are forming. Many of the molecules Townes listed in his 1955 talk have been discovered, along with an even larger number of other molecules. From observations of these molecules, particularly CO, we have learned an enormous amount about the conditions under which molecules can exist in the interstellar medium. Here we consider how these conditions lead to the formation of low-mass stars, and how this star formation in turn governs the structure of the molecular clouds in which most molecules are embedded. A fuller account of this work will be given elsewhere [3].
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
C. H. Townes, in IAU Symposium 4, Radio Astronomy, ed. H. C. van de Hulst (London: Cambridge University Press), p. 92 (1957).
A. C. Cheung, D. M. Rank, C. H. Townes, D. D. Thornton, and W. J. Welch, Phys. Rev. Lett. 21, 1701 (1968).
F. Bertoldi and C. F. McKee, in preparation (1995).
C. J. Lada and E. A. Lada, in The Formation and Evolution of Star Clusters, ed. Janes (ASP), p. 3 (1991).
E. A. Lada, N. J. I. Evans, D. L. DePoy, and I. Gatley, ApJ 371, 171 (1991).
E. A. Lada, ApJ 393, L25 (1992).
J. M. Carpenter, R. L. Snell, F. P. Schloerb, and M. F. Skrutskie, ApJ 407, 657 (1993).
E. A. Lada, K. M. Strom, and P. C. Myers, in Protostars and Planets III, eds. E. Levy and J. Lunine (Arizona), p. 245 (1993).
H. Zinnecker, M. J. McCaughrean, and B. A. Wilking, in Protostars and Planets III, eds. E. Levy and J. Lunine (Arizona), p. 429 (1993).
D. L. Block, T. R. Geballe, and J. E. Dyson, A&Amp;A 273, L41 (1993).
R. B. Loren, ApJ 338, 902 (1989).
R. B. Loren, ApJ 338, 925 (1989).
M. Gomez, L. Hartmann, S. J. Kenyon, and R. Hewett, AJ 105, 1927 (1993).
L. Blitz, in The Physics of Star Formation and Early Stellar Evolution, eds. C. J. Lada and N. D. Kylafis (Dordrecht: Kluwer), p. 3 (1991).
C.F. McKee, ApJ 345, 782 (1989).
G. Sundstrom et al., Science 263, 785 (1994).
F. Bertoldi and C. F. McKee, ApJ 395 140 (1992).
L. Blitz and F. H. Shu, ApJ 238, 148 (1980).
H. S- Liszt, ApJ 411, 720 (1993).
D. B. Sanders, N. Z. Scoville, R. P. J. Tilanus, Z. Wang, and S. Zhou, in Back to the Galaxy, ed. S. S. Holt and F. Verter ( New York: AIP ), p. 311 (1993).
P. C. Myers, in Molecular Clouds and Star Formation, ed. C. Yuan ( Singapore: World Press ) (1995).
R. B. Larson, MNRAS 194, 809 (1981).
P. M. Solomon, A. R. Rivolo, J. W. Barrett, and A. Yahil, ApJ 319, 730 (1987).
N. Z. Scoville and D. B. Sanders, in Interstellar Processes, eds. D. Hollenbach and H. Thronson ( Dordrecht: Reidel ), p. 21 (1987).
T. Mouschovias and L. Spitzer, ApJ 210, 326 (1976).
K. Tomisaka, S. Ikeuchin, and T. Nakamura, ApJ 335, 239 (1988).
P. C. Myers and A. A. Goodman, ApJ 326, L27 (1988).
B. G. Elmegreen, ApJ 299, 196 (1985).
R. G. Carlberg and R. E. Pudritz, MNRAS 247, 353 (1990).
J. L. Puget, in Fragmentation of Molecular Clouds and Star Formation, ed. E. Falgarone et al. ( Dordrecht: Kluwer ), p. 75 (1991).
C. A. Norman and J. Silk, ApJ 238, 158 (1980).
Y. Fukui, T. Iwata, A. Mizuno, J. Bally, and A. P. Lane, in Protostars and Planets III, eds. E. Levy and J. Lunine (University of Arizona Press), p. 603 (1993).
F. H. Shu, S. Lizano, S. P. Ruden, and J. Najita, ApJ 328, L19 (1988).
S. Cabrit and C. Bertout, A&A 261, 274 (1992).
L. Chernin, private communication.
F. H. Shu, F. C. Adams, and S. Lizano, ARA&Amp;A 25, 23 (1987).
T. Nakano, Fund. Cosmic Phys. 9, 139 (1984).
T. Mouschovias, ApJ 207, 141 (1976).
J. P. Williams and L. Blitz, ApJ, submitted (1995).
E. A. Lada and C. J. Lada, AJ 109, 1682 (1995).
K. M. Strom, S. E. Strom and K. M. Merrill, ApJ 412, 233 (1993).
C. F. Prosser, J. R. Stauffer, L. Hartmanry, D. R. Soderblom, B. F. Jones, M. W. Werner, and M. J. McCaughrean, ApJ 421, 517 (1994).
E. A. Lada, J. Bally and A. A. Stark, ApJ 368, 432 (1991).
Y. Fukui, K. Sugitani, T. Tabaka, A. Mizuno, H. Ogawa, and K. Kawabata, AJ 311, L85 (1986).
M. Margulis, C. J. Lada, and R. L. Snell, ApJ 333, 316 (1988).
J. A. Morgan, F. P. Schloerb, R. L. Snell, and J. Bally, ApJ 376, 618 (1991).
F. Bertoldi, C. F. McKee, and R. I. Klein, in Massive Stars: Their Lives in the Interstellar Medium, eds. J. Cassinelli and E. Churchwell (ASP Conf. Ser. 35), p. 129 (1993).
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1996 Springer-Verlag New York, Inc.
About this chapter
Cite this chapter
Bertoldi, F., McKee, C.F. (1996). Self-Regulated Star Formation in Molecular Clouds. In: Chiao, R.Y. (eds) Amazing Light. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-2378-8_5
Download citation
DOI: https://doi.org/10.1007/978-1-4612-2378-8_5
Publisher Name: Springer, New York, NY
Print ISBN: 978-1-4612-7521-3
Online ISBN: 978-1-4612-2378-8
eBook Packages: Springer Book Archive