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Journal article

Vigorous star formation in a bulge-dominated extremely red object at z=1.34

Abstract:: We present near-infrared (near-IR) spectroscopy of three extremely red objects (EROs) using the OHS/CISCO spectrograph at the Subaru Telescope. One target exhibits a strong emission line, which we identify as Ha at z = 1.34. Using new and existing ground-based optical and near-IR imaging, and archival Hubble Space Telescope imaging, we argue that this target is essentially an elliptical galaxy, with an old stellar population of around 4 × 10 11 M ...
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Publication status:: Published

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APA Style

Cotter, G., Simpson, C., & Bolton, R. (2005). Vigorous star formation in a bulge-dominated extremely red object at z=1.34. Monthly Notices of the Royal Astronomical Society, 360(2), 685–692.

MLA Style

Cotter, G., et al. “Vigorous Star Formation in a Bulge-Dominated Extremely Red Object at z=1.34.” Monthly Notices of the Royal Astronomical Society, vol. 360, no. 2, 2005, pp. 685–92.

Chicago Style

Cotter, G, C Simpson, and R Bolton. 2005. “Vigorous Star Formation in a Bulge-Dominated Extremely Red Object at z=1.34.” Monthly Notices of the Royal Astronomical Society 360 (2): 685–92.
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Publisher copy:: 10.1111/j.1365-2966.2005.09068.x

Authors

+ Cotter, G More by this author

Institution:

University of Oxford

Division:

MPLS

Department:

Physics

Sub department:

Astrophysics

Role:

Author

+ Simpson, C More by this author

Role:

Author

+ Bolton, R More by this author

Role:

Author

Bibliographic Details

Journal:: Monthly Notices of the Royal Astronomical Society
Volume:: 360
Issue:: 2
Pages:: 685-692
Publication date:: 2005-06-21
DOI:: 10.1111/j.1365-2966.2005.09068.x
EISSN:: 1365-2966
ISSN:: 0035-8711

Item Description

Language:: English
Keywords:: galaxies : evolution

galaxies : starburst

infrared : galaxies

cosmology : observations
Pubs id:: pubs:157378
UUID:: uuid:0aaa428d-d6a2-47c2-bb0a-d60fdbe6d046
Local pid:: pubs:157378
Source identifiers:: 157378
Deposit date:: 2012-12-19

Terms of use

Copyright date:: 2005

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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