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The Rest-Frame UV Spectrum of Elliptical...

Renzini, Alvio...

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The Rest-Frame UV Spectrum of Elliptical Galaxies at High Redshift by Renzini, Alvio ( Author )

Content Provider	Lemonjar Open Access
Publisher	N.A
Publication Date	09-08-2007
Summary	Beyond redshift ~1.4 the only spectral feature that allows one to get the redshift of passively evolving galaxies (PEG) with optical spectrographs is a characteristic structure due to a set of iron and magnesium lines lines at 2600-2850 Angstrom in the rest frame. The same feature permits also to estimate the time elapsed since the cessation of star formation. Current efforts at observing high redshift PEGs at the VLT and SUBARU telescopes are briefly reviewed.
ISBN	-
Item Type	Article
File Type	pdf
File Size	36.88 KB
Language	English
Subjects	-
Unlimited	MYR 0.00
Total read	-
URL	doi:10.1007/978-0-387-87621-4_1

Citation

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AMA 11th EditionReferences

Renzini, Alvio. The Rest-Frame UV Spectrum of Elliptical Galaxies at High Redshift. N.A. August 09, 2007. Accessed February 08, 2025. https://online.provdatabase.com/cite/15451

APA 7th EditionReferences

Renzini, Alvio. (2007). The Rest-Frame UV Spectrum of Elliptical Galaxies at High Redshift. N.A. https://online.provdatabase.com/cite/15451

Chicago 17th EditionReferences

Renzini, Alvio. The Rest-Frame UV Spectrum of Elliptical Galaxies at High Redshift. N.A. 2007. https://online.provdatabase.com/cite/15451

HarvardReferences

Renzini, Alvio. (2007). The Rest-Frame UV Spectrum of Elliptical Galaxies at High Redshift. [Online]. N.A. Available from: https://online.provdatabase.com/cite/15451. (Accessed 08 February 2025).

Harvard AustraliaReferences

Renzini, Alvio, 2007, The Rest-Frame UV Spectrum of Elliptical Galaxies at High Redshift, N.A, viewed 08 February 2025, <https://online.provdatabase.com/cite/15451>

MLA 9th EditionWorks Cited

Renzini, Alvio. The Rest-Frame UV Spectrum of Elliptical Galaxies at High Redshift. N.A, 2007. PROV Database, https://online.provdatabase.com/cite/15451.

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