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Molecular Studies of Herbig-Haro Objects

Published online by Cambridge University Press:  07 August 2017

Salvador Curiel
Salvador Curiel*
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden Street (MS 10) Cambridge, MA 02138

Abstract

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Recent ultraviolet, infrared, millimeter and centimeter-wavelength observations have revealed that HH objects are also sources of molecular line emission. Infrared observations have shown that H2 line emission in HH objects presents a wide and complex variety of morphologies, being in most of the cases similar to that observed at optical wavelengths. New high-angular resolution radio observations of molecular lines have revealed that small high-density condensations are frequently found in association with HH objects. Below, a brief review of molecular emission in HH objects is presented.

Type
Near Stellar Environments
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 373 - 378
Copyright
Copyright © Kluwer 1992 

References

REFERENCES

Bally, J., and Lane, A.P. 1991, in Astrophysics with Infrared arrays, ASP vol. 14, ed. Elston, R., p. 273–278.Google Scholar
Black, J.H., and van Dishoeck, 1987, Ap. J. , 322, 412.Google Scholar
Böhm, K., Bührke, Th., Raga, A., Brugel, E., Witt, A., and Mundt, R. 1987, Ap. J. , 316, 349.Google Scholar
Brand, P.W.J.L., Toner, M.P., Geballe, T.R., and Webster, A.S. 1989, MNRAS , 237, 1009.Google Scholar
Brugel, E.W. 1989, in ESO-Workshop on Low Mass Star Formation and Pre-Main Sequence Objects, ed. Reipurth, Bo, p. 311–329.Google Scholar
Bugel, E.W., Shull, J.M., and Seab, C.G. 1982, Ap. J. , 262, L35.Google Scholar
Burton, M.G., Brand, P.W.J.L., Geballe, T.R., and Webster, A.S. 1989, MNRAS , 236, 409.Google Scholar
Carr, J.S. 1990, Bull. AAS , 21, 1086.Google Scholar
Curiel, S. 1991, PhD Thesis, Universidad Nacional Autónoma de México. Google Scholar
Davis, C.J., Dent, W.R.F., and Bell Burnell, S.J. 1990, MNRAS , 244, 173.Google Scholar
Dopita, M.A., Binette, L., and Schwartz, R.D. 1982, Ap. J. , 261, 183.Google Scholar
Doyon, R., and Nadeau, D. 1988, Ap. J. , 334, 883.Google Scholar
Elias, J.H. 1980, Ap. J. , 241, 728.Google Scholar
Garden, R.P., Russell, A.P.G., and Burton, M.G. 1990, Ap. J. , 354, 232.Google Scholar
Hartigan, P., Curiel, S., and Raymond, J. 1989, Ap. J. (Letters) , 347, L31.Google Scholar
Hartigan, P., Curiel, S., and Raymond, J. 1991, in preparation.Google Scholar
Hartigan, P., Lada, C.J., Stocke, J., and Tapia, S. 1986, A. J. , 92, 1155.Google Scholar
Hartigan, P., Raymond, J., and Hartmann, L. 1987, Ap. J. , 316, 323.Google Scholar
Hartmann, L., and Raymond, J. 1984, Ap. J. , 276, 560.CrossRefGoogle Scholar
Harvey, P.M., Joy, M., Lester, D.F., and Wilking, B.A. 1986, Ap. J. , 301, 346.Google Scholar
Lane, A.P. 1989, in ESO-Workshop on Low Mass Star Formation and Pre-Main Sequence Objects, ed. Reipurth, Bo, p. 331–348.Google Scholar
Lane, A.P., and Bally, J. 1986, Ap. J. , 310, 820.Google Scholar
Lane, A.P., Bally, J., and Hartigan, P. 1991, in preparation.Google Scholar
Lenzen, R. 1988, Astr. Ap. , 190, 269.Google Scholar
Lightfoot, J.F., and Glencross, W.M. 1986, MNRAS , 221, 993.Google Scholar
Rudolph, A., and Welch, W.J. 1988, Ap. J. (Letters) , 326, L31.Google Scholar
Sandell, G., Zealey, W.J., Williams, P.M., Taylor, K., and Strey, J.V. 1987, Astr. Ap. , 182, 237.Google Scholar
Schwartz, R.D. 1983, Ann. Rev. Astr. Ap. , 21, 209.Google Scholar
Schwartz, R.D., Cohen, M., and Williams, P.M. 1987, Ap. J. , 322, 403.Google Scholar
Schwartz, R.D., Cohen, M., and Williams, P.M. 1988a, Ap. J. , 333, 1035.Google Scholar
Schwartz, R.D., Williams, P.M., Cohen, M., and Jennings, D.G. 1988b, Ap. J. (Letters) , 334, L99.Google Scholar
Shull, J.M., and Hollenbach, D.J. 1978, Ap. J. , 220, 525.Google Scholar
Solf, J., and Böhm, K.H. 1987, A. J. , 93, 1172.Google Scholar
Stapelfeldt, K.R., Beichman, C.A., Hester, J.J., Scoville, N.Z., and Gautier, T.N. III 1991, Ap. J. (Letters), , in press.Google Scholar
Strom, K.M., Strom, S.E., Wolff, S.C., Morgan, J., and Wenz, M. 1986, Ap. J. Suppl. , 62, 39.Google Scholar
Torrelles, J.M. 1990, in Atoms, Ions, and Molecules: New Results in Spectral Line Astrophysics, ASP vol. 16, eds. Haschick, A.D. and Ho, P.T.P., p. 257–268.Google Scholar
Torrelles, J.M., Ho, P.T.P., Rodríguez, L.F., Cantó, J., and Verdes, L. 1989, Ap. J. , 346, 756.Google Scholar
Wilking, B.A., Schwartz, R.D., Mundy, L.G., and Schultz, A.S.B. 1990, A. J. , 99, 344.Google Scholar
Wolfire, M.G., and Königl, A. 1991, Ap. J., in press.Google Scholar
Zealey, W.J., Williams, P.M., and Sandell, G. 1984, Astr. Ap. , 140, L31.Google Scholar
Zealey, W.J., Williams, P.M., Taylor, K.N., Storey, J.W., and Sandell, G. 1986, Astr. Ap. , 158, L9.Google Scholar
Zinnecker, H., Mundt, R., Geballe, T.R., and Zealey, W.J. 1989, Ap. J. , 342, 337.Google Scholar