MOND implications for spectral line profiles of shell galaxies:
shell formation history and mass-velocity scaling relations

J 2015

MOND implications for spectral line profiles of shell galaxies: shell formation history and mass-velocity scaling relations

BILEK, Michal; Bruno JUNGWIERT; Ivana EBROVA a Kateřina BARTOŠKOVÁ

Základní údaje

Originální název

MOND implications for spectral line profiles of shell galaxies: shell formation history and mass-velocity scaling relations

Autoři

BILEK, Michal; Bruno JUNGWIERT; Ivana EBROVA a Kateřina BARTOŠKOVÁ

Vydání

ASTRONOMY & ASTROPHYSICS, LES ULIS CEDEX A, EDP SCIENCES S A, 2015, 1432-0746

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10301 Atomic, molecular and chemical physics

Stát vydavatele

Francie

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL

Označené pro přenos do RIV

Ano

Kód RIV

RIV/00216224:14310/15:00093054

Organizační jednotka

Přírodovědecká fakulta

Klíčová slova anglicky

gravitation; galaxies: kinematics and dynamics; galaxies: peculiar; galaxies: elliptical

Štítky

AKR, rivok

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 17. 4. 2017 12:14, Ing. Andrea Mikešková

Anotace

V originále

Context. Many ellipticals are surrounded by round stellar shells probably stemming from minor mergers. A new method for constraining gravitational potential in elliptical galaxies has recently been suggested. It uses the spectral line profiles of these shells to measure the circular velocity at the edge of the shell and the expansion velocity of the shell itself. MOND is an alternative to the dark matter framework aiming to solve the missing mass problem. Aims. We study how the circular and expansion velocities behave in MOND for large shells. Methods. The asymptotic behavior for infinitely large shells is derived analytically. The applicability of the asymptotic results for finitely sized shells is studied numerically on a grid of galaxies modeled with Sersic spheres. Results. Circular velocity settles asymptotically at a value determined by the baryonic mass of the galaxy forming the baryonic Tully-Fisher relation known for disk galaxies. Shell expansion velocity also becomes asymptotically constant. The expansion velocities of large shells form a multibranched analogy to the baryonic Tully-Fisher relation, together with the galactic baryonic masses. For many - but not all - shell galaxies, the asymptotic values of these two types of velocities are reached under the effective radius. If MOND is assumed to work in ellipticals, then the shell spectra allow many details of the history to be revealed about the formation of the shell system, including its age. The results pertaining to circular velocities apply to all elliptical galaxies, not only those with shells.

Návaznosti

MUNI/A/0773/2013, interní kód MU

Název: Pokročilé problémy teoretické fyziky a astrofyziky

Investor: Masarykova univerzita, Pokročilé problémy teoretické fyziky a astrofyziky, DO R. 2020_Kategorie A - Specifický výzkum - Studentské výzkumné projekty

Citovat

BILEK, Michal; Bruno JUNGWIERT; Ivana EBROVA a Kateřina BARTOŠKOVÁ. MOND implications for spectral line profiles of shell galaxies: shell formation history and mass-velocity scaling relations. ASTRONOMY & ASTROPHYSICS. LES ULIS CEDEX A: EDP SCIENCES S A, 2015, roč. 575, March, s. "nestrankovano", 8 s. ISSN 1432-0746. Dostupné z: https://doi.org/10.1051/0004-6361/201424831.

@article{1368674,
   author = {Bilek, Michal and Jungwiert, Bruno and Ebrova, Ivana and Bartošková, Kateřina},
   article_location = {LES ULIS CEDEX A},
   article_number = {March},
   doi = {https://doi.org/10.1051/0004-6361/201424831},
   keywords = {gravitation; galaxies: kinematics and dynamics; galaxies: peculiar; galaxies: elliptical},
   language = {eng},
   issn = {1432-0746},
   journal = {ASTRONOMY & ASTROPHYSICS},
   title = {MOND implications for spectral line profiles of shell galaxies: shell formation history and mass-velocity scaling relations},
   url = {http://www.aanda.org/articles/aa/abs/2015/03/aa24831-14/aa24831-14.html},
   volume = {575},
   year = {2015}
}

TY  - JOUR
ID  - 1368674
AU  - Bilek, Michal - Jungwiert, Bruno - Ebrova, Ivana - Bartošková, Kateřina
PY  - 2015
TI  - MOND implications for spectral line profiles of shell galaxies: shell formation history and mass-velocity scaling relations
JF  - ASTRONOMY & ASTROPHYSICS
VL  - 575
IS  - March
SP  - "nestrankovano"
EP  - "nestrankovano"
PB  - EDP SCIENCES S A
SN  - 14320746
KW  - gravitation
KW  - galaxies: kinematics and dynamics
KW  - galaxies: peculiar
KW  - galaxies: elliptical
UR  - http://www.aanda.org/articles/aa/abs/2015/03/aa24831-14/aa24831-14.html
N2  - Context. Many ellipticals are surrounded by round stellar shells probably stemming from minor mergers. A new method for constraining gravitational potential in elliptical galaxies has recently been suggested. It uses the spectral line profiles of these shells to measure the circular velocity at the edge of the shell and the expansion velocity of the shell itself. MOND is an alternative to the dark matter framework aiming to solve the missing mass problem. Aims. We study how the circular and expansion velocities behave in MOND for large shells. Methods. The asymptotic behavior for infinitely large shells is derived analytically. The applicability of the asymptotic results for finitely sized shells is studied numerically on a grid of galaxies modeled with Sersic spheres. Results. Circular velocity settles asymptotically at a value determined by the baryonic mass of the galaxy forming the baryonic Tully-Fisher relation known for disk galaxies. Shell expansion velocity also becomes asymptotically constant. The expansion velocities of large shells form a multibranched analogy to the baryonic Tully-Fisher relation, together with the galactic baryonic masses. For many - but not all - shell galaxies, the asymptotic values of these two types of velocities are reached under the effective radius. If MOND is assumed to work in ellipticals, then the shell spectra allow many details of the history to be revealed about the formation of the shell system, including its age. The results pertaining to circular velocities apply to all elliptical galaxies, not only those with shells.
ER  -

BILEK, Michal; Bruno JUNGWIERT; Ivana EBROVA a Kateřina BARTOŠKOVÁ. MOND implications for spectral line profiles of shell galaxies: shell formation history and mass-velocity scaling relations. \textit{ASTRONOMY \&{} ASTROPHYSICS}. LES ULIS CEDEX A: EDP SCIENCES S A, 2015, roč.~575, March, s.~''nestrankovano'', 8 s. ISSN~1432-0746. Dostupné z: https://doi.org/10.1051/0004-6361/201424831.

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