text:   Dwarf Galaxies",13,"[""SO SO excited bc it's my first paper day!! We use a suite of isolated dwarf galaxy (FIRE) simulations to study stellar metallicity gradients and their origins: <LINK> <LINK>"", 'We predict that dwarf galaxies follow a gradient-strength-galaxy-age relationship such that galaxies with older stellar populations tend to have stronger (more negative) stellar metallicity gradients. https://t.co/rtvwu3QmxY', 'We also use published results for 10 existing Local Group dwarf galaxies to show that they, too, follow a VERY similar gradient-strength-galaxy-age relationship. https://t.co/oRmWjqyGCR', 'Interestingly, most of these observed galaxies are satellites of the MW while our simulated galaxies are ISOLATED systems... Yet they follow this very similar relationship!', 'This suggests that the environment of a dwarf galaxy likely plays a secondary role in shaping stellar metallicity gradients. Check the paper out to learn about what drives these gradients! https://t.co/2wLirxBaNF', ""I dedicate this paper to José A. Flores Velázquez and Perla Maritza Mercado. I wish they were both still here to celebrate with me but I know they're both proud ❤️❤️"", ""It's important to remember that none of this would be possible w/o support from the community around me. My thanks go out to my co-authors especially @jbprime and @jorgito__moreno. And thanks to @DarthLazar for always being willing to answer my endless onslaught of questions!"", '@j_tharindu thanks Tharindu!', '@astrochicana Muchísimas gracias!! 😊', '@astroarianna 💜💜💜', '@8minutesold Thank you!! 😃', '@ynxmonica Thanks Monica!! 😃', '@Naj_Astro Thanks Najmeh!!']",20,09,1529