Academic Journal

TO APPEAR IN THE ASTROPHYSICAL JOURNAL LETTERS Preprint typeset using L ATEX style emulateapj v. 04/03/99 FAR-ULTRAVIOLET EMISSION FROM ELLIPTICAL GALAXIES AT z = 0.33 1

التفاصيل البيبلوغرافية
العنوان: TO APPEAR IN THE ASTROPHYSICAL JOURNAL LETTERS Preprint typeset using L ATEX style emulateapj v. 04/03/99 FAR-ULTRAVIOLET EMISSION FROM ELLIPTICAL GALAXIES AT z = 0.33 1
المؤلفون: Thomas M. Brown, Henry C. Ferguson, Charles W. Bowers, Randy A. Kimble, R. Michael Rich
المساهمون: The Pennsylvania State University CiteSeerX Archives
المصدر: http://arxiv.org/pdf/astro-ph/0301364v1.pdf.
سنة النشر: 2003
المجموعة: CiteSeerX
الوصف: We present far-ultraviolet (far-UV) images of the rich galaxy cluster ZwCl1358.1+6245, taken with the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope (HST). When combined with archival HST observations, our data provide a measurement of the UV-to-optical flux ratio in 8 early-type galaxies at z = 0.33. Because the UV flux originates in a population of evolved, hot, horizontal branch (HB) stars, this ratio is potentially one of the most sensitive tracers of age in old populations – it is expected to fade rapidly with lookback time. We find that the UV emission in these galaxies, at a lookback time of 3.9 Gyr, is significantly weaker than it is in the current epoch, yet similar to that in galaxies at a lookback time of 5.6 Gyr. Taken at face value, these measurements imply different formation epochs for the massive ellipticals in these clusters, but an alternative explanation is a “floor ” in the UV emission due to a dispersion in the parameters that govern HB morphology.
نوع الوثيقة: text
وصف الملف: application/pdf
اللغة: English
Relation: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.3255; http://arxiv.org/pdf/astro-ph/0301364v1.pdf
الاتاحة: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.3255
http://arxiv.org/pdf/astro-ph/0301364v1.pdf
Rights: Metadata may be used without restrictions as long as the oai identifier remains attached to it.
رقم الانضمام: edsbas.752C586B
قاعدة البيانات: BASE