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The circumnuclear environment of the peculiar galaxy NGC3310
Elena Kirilovsky Terlevich
ROBERTO GIOVANNI TERLEVICH AFONSO
Acceso Abierto
Atribución-NoComercial-SinDerivadas
H🇮🇮 regions
Galaxies: individual: NGC3310
Galaxies: kinematics and dynamics
Galaxies: starburst
Galaxies: star clusters
Gas and star velocity dispersions have been derived for eight circumnuclear star-forming regions (CNSFRs) and the nucleus of the spiral galaxy NGC3310 using high-resolution spectroscopy in the blue and far red. Stellar velocity dispersions have been obtained from the Ca 🇮🇮 triplet in the near-IR, using cross-correlation techniques, while gas velocity dispersions have been measured by Gaussian fits to the Hβ λ4861Å and [O 🇮🇮🇮] λ5007Å emission lines. The CNSFR stellar velocity dispersions range from 31 to 73 km s⁻¹. These values, together with the sizes measured on archival Hubble Space Telescope images, yield upper limits to the dynamical masses for the individual star clusters between 1.8 and 7.1 × 10⁶M⊙, for the whole CNSFR between 2 × 10⁷ and 1.4 × 10⁸M⊙, and 5.3 × 10⁷M⊙, for the nucleus inside the inner 14.2 pc. The masses of the ionizing stellar population responsible for the H🇮🇮 region gaseous emission have been derived from their published Hα luminosities and are found to be between 8.7 × 10⁵ and 2.1 × 10⁶M⊙ for the star-forming regions and 2.1 × 10⁵M⊙ for the galaxy nucleus; they therefore constitute between 1 and 7 per cent of the total dynamical mass. The ionized gas kinematics is complex; two different kinematical components seem to be present as evidenced by different linewidths and Doppler shifts.
Monthly Notices of the Royal Astronomical Society
2010
Artículo
Inglés
Estudiantes
Investigadores
Público en general
Hagele, Guillermo F., et al., (2010), The circumnuclear environment of the peculiar galaxy NGC3310, Monthly Notices of the Royal Astronomical Society, Vol. 402(2):1005 - 1026
ASTRONOMÍA Y ASTROFÍSICA
Versión aceptada
acceptedVersion - Versión aceptada
Aparece en las colecciones: Artículos de Astrofísica

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