Age Dependence of Non-Radiative Heating in Stellar Chromospheres: Cycle 2

Details Age Dependence of Non-Radiative Heating in Stellar Chromospheres: Cycle 2 Age Dependence of Non-Radiative Heating in Stellar Chromospheres: Cycle 2

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.3950w&link_type=abstract

HST Proposal ID #3950

Physics

Hst Proposal Id #3950

Scientific paper

We propose to continue observations of a sample of late A/ early F
dwarfs in the Pleiades, UMa and Hyades clusters, and in the field, to
study the inception of chromospheric emission as a function of stellar
temperature and age. The scope of this program has decreased with time:
all we have time to do this cycle is alpha Aql, A7 IV-V.

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