Optical integral field spectroscopy of NGC 5850

M. Bremer; J. Scharwächter; A. Eckart; J. Zuther; S. Fischer; M. Valencia-S

doi:10.1088/1742-6596/372/1/012054

Optical integral field spectroscopy of NGC 5850

M. Bremer^*, J. Scharwächter, A. Eckart, J. Zuther, S. Fischer, M. Valencia-S

^*Corresponding author for this work

Research output: Contribution to journal › Conference article › peer-review

2 Citations (Scopus)

Abstract

Here we present the preliminary results of the analysis of VIMOS observations of the central 4.5 kpc of the double-barred galaxy NGC 5850. We use optical diagnostic diagrams to study the main ionization mecahnism across the field of view confirming the LINER nature in the continuum peak location. Also a star-forming (SF) region is found close to it (0.46kpc), a second SF region is located east of the center (1.6kpc). Further the data reveals a complex nuclear gas kinematics which is likely to be dominated by the secondary bar.

Original language	English
Article number	012054
Journal	Journal of Physics: Conference Series
Volume	372
DOIs	https://doi.org/10.1088/1742-6596/372/1/012054
Publication status	Published - 2012
Event	Astronomy at High Angular Resolution 2011: The Central Kiloparsec in Galactic Nuclei, AHAR 2011 - Bad Honnef, Germany Duration: 29 Aug 2011 → 2 Sept 2011

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10.1088/1742-6596/372/1/012054

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title = "Optical integral field spectroscopy of NGC 5850",

abstract = "Here we present the preliminary results of the analysis of VIMOS observations of the central 4.5 kpc of the double-barred galaxy NGC 5850. We use optical diagnostic diagrams to study the main ionization mecahnism across the field of view confirming the LINER nature in the continuum peak location. Also a star-forming (SF) region is found close to it (0.46kpc), a second SF region is located east of the center (1.6kpc). Further the data reveals a complex nuclear gas kinematics which is likely to be dominated by the secondary bar.",

author = "M. Bremer and J. Scharw{\"a}chter and A. Eckart and J. Zuther and S. Fischer and M. Valencia-S",

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language = "English",

volume = "372",

journal = "Journal of Physics: Conference Series",

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note = "Astronomy at High Angular Resolution 2011: The Central Kiloparsec in Galactic Nuclei, AHAR 2011 ; Conference date: 29-08-2011 Through 02-09-2011",

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TY - JOUR

T1 - Optical integral field spectroscopy of NGC 5850

AU - Bremer, M.

AU - Scharwächter, J.

AU - Eckart, A.

AU - Zuther, J.

AU - Fischer, S.

AU - Valencia-S, M.

PY - 2012

Y1 - 2012

N2 - Here we present the preliminary results of the analysis of VIMOS observations of the central 4.5 kpc of the double-barred galaxy NGC 5850. We use optical diagnostic diagrams to study the main ionization mecahnism across the field of view confirming the LINER nature in the continuum peak location. Also a star-forming (SF) region is found close to it (0.46kpc), a second SF region is located east of the center (1.6kpc). Further the data reveals a complex nuclear gas kinematics which is likely to be dominated by the secondary bar.

AB - Here we present the preliminary results of the analysis of VIMOS observations of the central 4.5 kpc of the double-barred galaxy NGC 5850. We use optical diagnostic diagrams to study the main ionization mecahnism across the field of view confirming the LINER nature in the continuum peak location. Also a star-forming (SF) region is found close to it (0.46kpc), a second SF region is located east of the center (1.6kpc). Further the data reveals a complex nuclear gas kinematics which is likely to be dominated by the secondary bar.

UR - https://www.scopus.com/pages/publications/84865646773

U2 - 10.1088/1742-6596/372/1/012054

DO - 10.1088/1742-6596/372/1/012054

M3 - Conference article

AN - SCOPUS:84865646773

SN - 1742-6588

VL - 372

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

M1 - 012054

T2 - Astronomy at High Angular Resolution 2011: The Central Kiloparsec in Galactic Nuclei, AHAR 2011

Y2 - 29 August 2011 through 2 September 2011

ER -

Optical integral field spectroscopy of NGC 5850

Abstract

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