{ "id": "1901.04573", "version": "v1", "published": "2019-01-14T21:33:02.000Z", "updated": "2019-01-14T21:33:02.000Z", "title": "Rejuvenated galaxies with very old bulges at the origin of the bending of the main sequence and of the \"green valley\"", "authors": [ "Chiara Mancini", "Emanuele Daddi", "Stéphanie Juneau", "Alvio Renzini", "Giulia Rodighiero", "Michele Cappellari", "Lucía Rodríguez-Muñoz", "Daizhong Liu", "Maurilio Pannella", "Ivano Baronchelli", "Alberto Franceschini", "Pietro Bergamini", "Chiara D'Eugenio", "Annagrazia Puglisi" ], "comment": "23 pages, 17 figures, submitted to MNRAS", "categories": [ "astro-ph.GA" ], "abstract": "We investigate the nature of star-forming galaxies with reduced specific star formation rate (sSFR) and high stellar masses, those `green valley' objects that seemingly cause a reported bending, or flattening, of the star-forming main sequence. The fact that such objects host large bulges recently led some to suggest that the internal formation of bulges was a late event that induced the sSFRs of massive galaxies to drop in a slow downfall, and thus the main sequence to bend. We have studied in detail a sample of 10 galaxies at $0.45