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On the Angular Correlation Functions of the Hubble Deep Field

Published online by Cambridge University Press:  25 May 2016

Boudewijn F. Roukema
Boudewijn F. Roukema*
Affiliation:
National Observatory of Japan, Mitaka, 181 Tokyo, Japan, email: [email protected]

Extract

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Roukema & Valls-Gabaud (1997) reinforce the conclusion of Colley et al. (1996, 1997) that the Hubble Deep Field (HDF) “galaxies” are probably star-forming regions, not “building-blocks”.

Type
Deep Fields & Evolution
Information
Symposium - International Astronomical Union , Volume 186: Galaxy Interactions at High and Low Redshift , 1999 , pp. 485
Copyright
Copyright © Kluwer 1999 

References

Colley, W.N., Rhoads, J.E., Ostriker, J.P. & Spergel, D.N. 1996, ApJ, 473, L63 Google Scholar
Colley, W.N., Gnedin, O.Y., Ostriker, J.P. & Rhoads, J.E. 1997, ApJ, 488, 579 Google Scholar
Groth, E.J. & Peebles, P.J.E. 1977, ApJ, 217, 385 CrossRefGoogle Scholar
Limber, D.N. 1953, ApJ, 117, 134 Google Scholar
Ogawa, T., Roukema, B.F., Yamashita, K. 1997, ApJ, 484, 53 Google Scholar
Roukema, B.F., Peterson, B.A., Quinn, P.J. & Rocca-Volmerange, B. 1998, MNRAS, in press (astro-ph/9707294) Google Scholar
Roukema, B.F. & Valls-Gabaud, D. 1997, ApJ, 488, 524 Google Scholar