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Ultra-Luminous X-ray Sources in Haro 11 and the Role of X-ray Binaries in Feedback in Lyman-alpha Emitting Galaxies
A. H. Prestwich, F. Jackson, P. Kaaret +4
Lyman Break Analogs (LBA) are local proxies of high-redshift Lyman Break Galaxies (LBG). Studies of nearby starbursts have shown that Lyman continuum and line emission are absorbed…
Linking Stellar Coronal Activity and Rotation at 500 Myr: A Deep Chandra Observation of M37
Alejandro Núñez, Marcel A. Agüeros, Kevin R. Covey +9
Empirical calibrations of the stellar age-rotation-activity relation (ARAR) rely on observations of the co-eval populations of stars in open clusters. We used the Chandra X-ray Obs…
Stellar Activity and Coronal Heating: an overview of recent results
Paola Testa, Steve Saar, Jeremy Drake
Observations of the coronae of the Sun and of solar-like stars provide complementary information to advance our understanding of stellar magnetic activity, and of the processes lea…
Internetwork chromospheric bright grains observed with IRIS
Juan Martínez-Sykora, Luc Rouppe van der Voort, Mats Carlsson +18
The Interface Region Imaging Spectrograph (IRIS) reveals small-scale rapid brightenings in the form of bright grains all over coronal holes and the quiet sun. These bright grains a…
Steps toward a high precision solar rotation profile: Results from SDO/AIA coronal bright point data
Davor Sudar, Ivica Skokić, Roman Brajša +1
Coronal bright points (CBP) are ubiquitous small brightenings in the solar corona associated with small magnetic bipoles. We derive the solar differential rotation profile by traci…