DOI: 10.1017/s0074180900233901. Observable Properties of Passively-Evolving Galaxies at High Redshift

Observable Properties of Passively-Evolving Galaxies at High Redshift

10.1017/s0074180900233901

Crossref journal-article

Cambridge University Press (CUP)

Symposium - International Astronomical Union (56)

Abstract

There are evidenves which suggest that many of the early-type galaxies in rich cluster environment formed at fairly high redshift, z > 2. If the galaxies formed at such early epoch have experienced no intensive star-formation events, their photometric properties can be traced with less ambiguity by using the stellar evolutionary sinthesis models. Here we demonstrate what conspicuous feature can be observed for those passively-evolving galaxies at high redshift and how we can constrain the epoch and period of their formation.

Bibliography

Yamada, T., & Arimoto, N. (1996). Observable Properties of Passively-Evolving Galaxies at High Redshift. Symposium - International Astronomical Union, 171, 472â472.

Authors 2

Toru Yamada (first)
Nobuo Arimoto (additional)

References 0 Referenced 1

None

Dates

Type	When
Created	9 years, 1 month ago (July 20, 2016, 12:25 a.m.)
Deposited	6 years, 2 months ago (June 6, 2019, 7:55 a.m.)
Indexed	3 years, 5 months ago (March 30, 2022, 5:21 p.m.)
Issued	29 years, 8 months ago (Jan. 1, 1996)
Published	29 years, 8 months ago (Jan. 1, 1996)
Published Online	9 years, 3 months ago (May 25, 2016)
Published Print	29 years, 8 months ago (Jan. 1, 1996)

Funders 0

None

BibTeX

@article{Yamada_1996, title={Observable Properties of Passively-Evolving Galaxies at High Redshift}, volume={171}, ISSN={0074-1809}, url={http://dx.doi.org/10.1017/s0074180900233901}, DOI={10.1017/s0074180900233901}, journal={Symposium - International Astronomical Union}, publisher={Cambridge University Press (CUP)}, author={Yamada, Toru and Arimoto, Nobuo}, year={1996}, pages={472–472} }

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