Kavli Affiliate: Gregory Herczeg | Summary:The proliferation of high time-resolution and decades-long monitoring of classical T Tauri stars provides a vast opportunity to test the variability of the star-disk connections. However, most monitoring surveys use single broad-band filters, which makes the conversion of photometric variability into accretion rate difficult. In this study, we analyze accretion […]
Continue.. The mass distribution of clumpy accretion onto the nearby young star TW Hya