OSCILLATING RED GIANTS OBSERVED DURING CAMPAIGN 1 OF THE KEPLER K2 MISSION: NEW PROSPECTS FOR GALACTIC ARCHAEOLOGY

ABSTRACT NASA's re-purposed Kepler mission-dubbed K2-has brought new scientific opportunities that were not anticipated for the original Kepler mission. One science goal that makes optimal use of K2's capabilities, in particular its 360° ecliptic field of view, is galactic archaeology-the...

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Published in:	Astrophysical journal. Letters 2015-08, Vol.809 (1), p.1-6
Main Authors:	Stello, Dennis, Huber, Daniel, Sharma, Sanjib, Johnson, Jennifer, Lund, Mikkel N., Handberg, Rasmus, Buzasi, Derek L., Aguirre, Victor Silva, Chaplin, William J., Miglio, Andrea, Pinsonneault, Marc, Basu, Sarbani, Bedding, Tim R., Bland-Hawthorn, Joss, Casagrande, Luca, Davies, Guy, Elsworth, Yvonne, Garcia, Rafael A., Mathur, Savita, Mauro, Maria Pia Di, Mosser, Benoit, Schneider, Donald P., Serenelli, Aldo, Valentini, Marica
Format:	Article
Language:	eng
Subjects:	Astronomical models Evolutionary Fossils Galaxies Galaxy: evolution Galaxy: stellar content Galaxy: structure Missions Oscillations Photometry Red giant stars stars: fundamental parameters stars: oscillations
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Summary:	ABSTRACT NASA's re-purposed Kepler mission-dubbed K2-has brought new scientific opportunities that were not anticipated for the original Kepler mission. One science goal that makes optimal use of K2's capabilities, in particular its 360° ecliptic field of view, is galactic archaeology-the study of the evolution of the Galaxy from the fossil stellar record. The thrust of this research is to exploit high-precision, time-resolved photometry from K2 in order to detect oscillations in red giant stars. This asteroseismic information can provide estimates of stellar radius (hence distance), mass, and age of vast numbers of stars across the Galaxy. Here we present the initial analysis of a subset of red giants, observed toward the north galactic gap, during the mission's first full science campaign. We investigate the feasibility of using K2 data for detecting oscillations in red giants that span a range in apparent magnitude and evolutionary state (hence intrinsic luminosity). We demonstrate that oscillations are detectable for essentially all cool giants within the range ∼1.9-3.2. Our detection is complete down to , which results in a seismic sample with little or no detection bias. This sample is ideally suited to stellar population studies that seek to investigate potential shortcomings of contemporary Galaxy models.
ISSN:	2041-8205 2041-8213