Please note that eDoc will be permanently shut down in the first quarter of 2021!      Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ
Home Search Quick Search Advanced Fulltext Browse Collections Persons My eDoc Session History Login Name: Password: Documentation Help Support Wiki Direct access to document ID:	Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents ID: 660804.0, MPI für Astronomie / Publikationen_mpia Dwarfs gobbling dwarfs: A stellar tidal stream around NGC 4449 and hierarchical galaxy formation on small scales Authors: Martínez-Delgado, D.; Romanowsky, A. J.; Gabany, R. J.; Annibali, F.; Arnold, J. A.; Fliri, J.; Zibetti, S.; van der Marel, R. P.; Rix, H.-W.; Chonis, T. S.; Carballo-Bello, J. A.; Aloisi, A.; Macciò, A. V.; Gallego-Laborda, J.; Brodie, J. P.; Merrifield, M. R. Date of Publication (YYYY-MM-DD): 2012 Journal Abbrev.: The Astrophysical Journal Letters Volume: 748 Issue / Number: 2 Start Page: id. L24 Audience: Not Specified Abstract / Description: A candidate diffuse stellar substructure was previously reported in the halo of the nearby dwarf starburst galaxy NGC 4449 by Karachentsev et al. We map and analyze this feature using a unique combination of deep integrated-light images from the BlackBird 0.5 m telescope, and high-resolution wide-field images from the 8 m Subaru Telescope, which resolve the nebulosity into a stream of red giant branch stars, and confirm its physical association with NGC 4449. The properties of the stream imply a massive dwarf spheroidal progenitor, which after complete disruption will deposit an amount of stellar mass that is comparable to the existing stellar halo of the main galaxy. The stellar mass ratio between the two galaxies is ~1:50, while the indirectly measured dynamical mass ratio, when including dark matter, may be ~1:10-1:5. This system may thus represent a "stealth" merger, where an infalling satellite galaxy is nearly undetectable by conventional means, yet has a substantial dynamical influence on its host galaxy. This singular discovery also suggests that satellite accretion can play a significant role in building up the stellar halos of low-mass galaxies, and possibly in triggering their starbursts. Free Keywords: galaxies: dwarf; galaxies: evolution; galaxies: interactions; galaxies: structure External Publication Status: published Document Type: Article Communicated by: N. N. Affiliations: MPI für Astronomie Identifiers: URL:http://cdsads.u-strasbg.fr/abs/2012ApJ...748L..24M The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.