Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...468l...9m&link_type=abstract
Astrophysical Journal Letters v.468, p.L9
Astronomy and Astrophysics
Astronomy
37
Galaxies: Evolution, Galaxies: Individual Alphanumeric: Mtm 095355+54528, Cosmology: Observations, Infrared: Galaxies
Scientific paper
We recently used narrowband infrared imaging to discover an H alpha -emitting galaxy at a redshift of z = 2.5 (Malkan, Teplitz, & McLean 1995). Optical spectroscopy with the Keck-I telescope reveals a spectrum of both strong narrow emission lines, especially Ly alpha and the stellar and interstellar absorption lines characteristic of young starbursts, at a redshift of 2.498. This galaxy has a current star formation rate of 10--100 Msolar yr-1 (the uncertainty depending mostly on reddening corrections), and should evolve into a normal galaxy with a present-day luminosity of L* or less. Combining deep optical imaging with our previous infrared photometry, we obtain an accurate VIJHK energy distribution which strongly constrains the evolutionary status of this object. The best model is a burst of star formation that started no earlier than z ~ 5.5. Therefore, this young galaxy is probably being seen during its initial episode of star formation, and meets our operational definition of a protogalaxy. In addition, further narrow-band infrared imaging of this region has revealed a close pair of fainter H alpha -emitting galaxies which lie within 500 kpc of the first galaxy. Their high H alpha luminosities and bluer colors suggest that they are seen even closer to the peak of their initial epochs of star formation. We propose that all three objects are part of a young galaxy cluster at z = 2.5.
Malkan Matthew A.
McLean Ian S.
Teplitz Harry
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