Summary
The current observational scenario pertaining to the study of low-mass star formation is discussed together with the evolutionary sequence that such a scenario seems to suggest. The opportunities offered by the spectrometers on board of the ISO satellite for improving our understanding of the involved physical processes are then discussed.
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References
Scientific Capabilities of the ISO Payload, ISO-SSD-8805, Draft 3.0, Space Science Department, ESTEC, Noordwijk, the Netherlands (October 1990).
ISO INFO, published by Space Science Department, ESTEC, Noordwijk, the Netherlands.
P. Saraceno:Nuovo Saggiatore,4, 19 (1988).
P. Clegg:Nuovo Cimento C,13, 249 (1990).
P. Saraceno, D. Lorenzetti andC. Ceccarelli (Editors):Proceeding of the workshop Spettroscopia con ISO, held in Frascati 17–19 February 1988.
C. J. Lada andB. A. Wilking:Astrophys. J.,287, 610 (1984).
F. Berrilli, C. Ceccarelli, R. Liseau, D. Lorenzetti, P. Saraceno andL. Spinoglio:Mon. Not. R. Astron. Soc.,237, 1 (1989).
I. Iben:Astrophys. J.,141, 993 (1965).
M. Cohen andL. V. Kuhi:Astrophys. J. Suppl. Ser.,41, 743 (1979).
P. J. Benson andP. C. Myers:Astrophys. J. Suppl. Ser.,71, 89 (1989).
C. A. Beichman, P. C. Myers, J. P. Emerson, S. Harris, R. Mathieu, P. J. Benson andR. E. Jennings:Astrophys. J.,307, 337 (1986).
C. K. Walker, F. C. Adams andC. J. Lada:Astrophys. J.,349, 515 (1990).
P. G. Mezger, J. E. Wink andR. Zylka:Astron. Astrophys.,228, 95 (1990).
F. O. Clark:Astrcm. Astrophys.,180, L1 (1987).
G. A. Fuller andP. C. Myers:Physical Processes in Interstellar Clouds, edited by G. E. Morfill and M. Sholer (Reidel Publishing Company, 1987), p. 137.
S. Terebey, S. N. Vogel andP. C. Myers:Astrophys. J.,340, 472 (1989).
F. C. Adams, C. J. Lada andF. H. Shu:Astrophys. J.,312, 788 (1987).
P. C. Myers, M. Heyer, R. L. Snell andP. F. Goldsmith:Astrophys. J.,324, 907 (1988).
M. Cohen, J. P. Emerson andG. Fuller:Astrophys. J.,339, 455 (1990).
S. Rucinski:Astron. J.,90, 2321 (1985).
M. Cohen, J. P. Emerson andC. A. Beichmann:Astrophys. J.,339, 455 (1989).
D. A. Weintraub, G. Sandell andW. D. Duncan:Astrophys. J.,340, L69 (1989).
S. V. W. Beckwith, A. Sargent, R. S. Chini andR. Gusten:Astron. J.,99, 924 (1990).
F. C. Adams, J. P. Emerson andG. Fuller:Astrophys. J.,357, 606 (1990).
P. Bastien andF. Menard:Astrophys. J.,364, 232 (1990).
S. Edwards, S. Cabrit, S. E. Strom, I. Heyer, K. M. Strom andE. Anderson:Astrophys. J.,321, 473 (1987).
D. Lynden-Bell andJ. Pringle:Mon. Not. R. Astron. Soc.,168, 603 (1974).
C. Bertout, G. Basri andJ. Bouvier:Astrophys. J.,330, 350 (1988).
B. A. Wilking, C. J. Lada andE. T. Young:Astrophys. J.,340, 823 (1989).
P. C. Myers, G. A. Fuller, R. D. Mathieu, C. A. Beichman, P. J. Benson, R. E. Schild andJ. P. Emerson:Astrophys. J.,319, 340 (1987).
S. J. Kenyon, L. W. Hartmann, K. M. Strom andS. E. Strom:Astron. J.,99, 869 (1990).
S. Stahler, F. H. Shu andR. E. Taam:Astrophys. J.,241, 637 (1980).
D. Hollenbach, M. Werner andE. E. Salpeter:Astrophys. J,163, 165 (1971).
M. Jura:Astrophys. J,197, 575 (1975).
F. Palla andH. Zinnecker: inStarburst and Galaxy Evolution, edited by T. X. Thuanet al., Editions Frontieres (1987), p. 533.
S. W. Stahler:Publ. Astron. Soc. Pac.,98, 1081 (1986).
S. W. Stahler, F. H. Shu andR. E. Taam:Astrophys. J.,241, 637 (1980).
S. Lizano andF. H. Shu:Astrophys. J.,342, 834 (1989).
F. H. Shu, S. Lizano andF. C. Adams: inStar Forming Regions, IAU Symposium 115, edited by M. Peimbert and J. Jungaku (Dordrech, Reidel, 1987), p. 417.
T. Ch. Mouschovias: inPhysical Processes in Interstellar Clouds, edited by G. E. Morfill and M. Scholer (Reidel Publishing Company, 1987), p. 453.
L. Mestel:Protostars and Planets II, edited by D. C. Block and M. S. Matthews University of Arizona, p. 320.
K. H. Winkler andM. J. Newman:Astrophys. J.,236, 201 (1980).
F. C. Adams:Astrophys. J.,363, 578 (1990).
F. C. Adams andF. H. Shu:Astrophys. J.,296, 655 (1985).
P. Bodenheimer, M. Rozyczka, H. W. Yorke andJ. E. Tohline: inFormation and Evolution of Low-mass Stars, edited by A. K. Dupree and M.T.V.T. Lago,Nato ASI Series, Vol. 241, (1988), p. 139.
T. Nakano:Fund. Cosm. Phys.,9, 139 (1984).
F. H. Shu, F. C. Adams andS. Lizano:Annu. Rev. Astron. Astrophys.,25, 23(1987).
F. D. Kahn:Astron. Astrophys.,37, 149 (1974).
H. W. Yorke andE. Krugel:Astron. Astrophys.,85, 215 (1977).
C. G. Wynn-Williams:Annu. Rev. Astron. Astrophys.,20, 587 (1982).
C. J. Lada: inStar Forming Regions IAU Symposium 115, edited by M. Peimbert and J. Jungaku (Dordrech, Reidel)115 (1987), p. 1.
R. H. Hildebrand:Q. J. R. Astron. Soc.,24, 267 (1983).
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Saraceno, P., Ceccarelli, C., Cerulli, P. et al. ISO spectroscopy: the study of low-mass star formation. Nouv Cim C 15, 1021–1032 (1992). https://doi.org/10.1007/BF02506693
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DOI: https://doi.org/10.1007/BF02506693