BILEK, Michal, JC. CUILLANDRE, S. GWYN, Ivana EBROVA, Kateřina BARTOŠKOVÁ, Bruno JUNGWIERT and Lucie JÍLKOVÁ. Deep imaging of the shell elliptical galaxy NGC3923 with MegaCam. ASTRONOMY & ASTROPHYSICS. LES ULIS CEDEX A: EDP SCIENCES S A, 2016, vol. 588, April, p. "nestrankovano", 12 pp. ISSN 1432-0746. Available from: https://dx.doi.org/10.1051/0004-6361/201526608.
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Basic information
Original name Deep imaging of the shell elliptical galaxy NGC3923 with MegaCam
Authors BILEK, Michal (203 Czech Republic, guarantor), JC. CUILLANDRE (250 France), S. GWYN (124 Canada), Ivana EBROVA (203 Czech Republic), Kateřina BARTOŠKOVÁ (203 Czech Republic, belonging to the institution), Bruno JUNGWIERT (203 Czech Republic) and Lucie JÍLKOVÁ (203 Czech Republic).
Edition ASTRONOMY & ASTROPHYSICS, LES ULIS CEDEX A, EDP SCIENCES S A, 2016, 1432-0746.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10301 Atomic, molecular and chemical physics
Country of publisher France
Confidentiality degree is not subject to a state or trade secret
Impact factor Impact factor: 5.014
RIV identification code RIV/00216224:14310/16:00093056
Organization unit Faculty of Science
Doi http://dx.doi.org/10.1051/0004-6361/201526608
UT WoS 000373207800089
Keywords in English galaxies: peculiar; galaxies: elliptical and lenticular; galaxies: individual: NGC 3923; galaxies: photometry; techniques: image processing; gravitation
Tags AKR, rivok
Tags International impact, Reviewed
Changed by Changed by: Ing. Andrea Mikešková, učo 137293. Changed: 31/3/2017 12:12.
Abstract
Context. The elliptical galaxy NGC3923 is known to be surrounded by a number of stellar shells, probable remnants of an accreted galaxy. Despite its uniqueness, the deepest images of its outskirts come from the 1980s. On the basis of the modified Newtonian dynamics (MOND), it has recently been predicted that a new shell lies in this region. Aims. We obtain the deepest image ever of the galaxy, map the tidal features in it, and search for the predicted shell. Methods. The image of the galaxy was taken by the MegaCam camera at the Canada-France-Hawaii Telescope in the g'-band. It reached the surface-brightness limit of 29 mag arcsec(-2). In addition, we reanalyzed an archival HST image of the galaxy. Results. We detected up to 42 shells in NGC3923. This is by far the highest number among all shell galaxies. We present the description of the shells and other tidal features in the galaxy. A probable progenitor of some of these features was discovered. The shell system likely originates from two or more progenitors. The predicted shell was not detected, but the new image revealed that the prediction was based on incorrect assumptions and poor data.
Links
MUNI/A/1110/2014, interní kód MUName: Pokročilé problémy astrofyziky, teoretické fyziky a fyzikálního vzdělávání
Investor: Masaryk University, Category A
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