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    STAR FORMATION RATE AND AGN IN BARRED GALAXIES

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    https://www.riss.kr/link?id=A104662971

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    We investigate the dependence of star formation rate and Active Galaxy Nuclei (AGN) frequency on the bar properties, especially the bar strength, using SDSS DR6. To better represent the bar strength, we divided the bars into 6 classes according to their length and axial ratios. There seems to be a fairly good correlation between the star formation rate derived from Hα emission lines and the bar strength, whereas there is no apparent correlation between the AGN activity and the bar strength. We interpret that the former correlation is due to the dependence of bar-driven gas inflow on the strength of bar. The lack of correlation between AGN and bar properties suggests that the accretion of gas onto a supermassive black hole(SMBH) is regulated by the interplay between the bar and SMBH. The frequency of AGN seems to be dependent on the background density but the star formation rate does not. It suggests that star formation is a localized phenomenon that is mostly determined by the gas density in a galaxy, while AGN activity is more closely related to the host property such as mass and luminosity that are thought to be dependent on the environment through the density-luminosity relation.
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    We investigate the dependence of star formation rate and Active Galaxy Nuclei (AGN) frequency on the bar properties, especially the bar strength, using SDSS DR6. To better represent the bar strength, we divided the bars into 6 classes according to th...

    We investigate the dependence of star formation rate and Active Galaxy Nuclei (AGN) frequency on the bar properties, especially the bar strength, using SDSS DR6. To better represent the bar strength, we divided the bars into 6 classes according to their length and axial ratios. There seems to be a fairly good correlation between the star formation rate derived from Hα emission lines and the bar strength, whereas there is no apparent correlation between the AGN activity and the bar strength. We interpret that the former correlation is due to the dependence of bar-driven gas inflow on the strength of bar. The lack of correlation between AGN and bar properties suggests that the accretion of gas onto a supermassive black hole(SMBH) is regulated by the interplay between the bar and SMBH. The frequency of AGN seems to be dependent on the background density but the star formation rate does not. It suggests that star formation is a localized phenomenon that is mostly determined by the gas density in a galaxy, while AGN activity is more closely related to the host property such as mass and luminosity that are thought to be dependent on the environment through the density-luminosity relation.

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    참고문헌 (Reference)

    1 형식, "시이펏 은하 NGC 5728의 OASIS 분광 영상" 한국지구과학회 27 (27): 569-578, 2006

    2 Donas, J., "Ultraviolet Observations and Starformation Rate in Galaxies" 180 : 12-26, 1987

    3 Kewley, L.J., "Theoretical Modeling of Starburst Galaxies" 556 : 121-140, 2001

    4 Ho, L.C, "The Influence of Bars on Nuclear Activity" 487 : 591-602, 1997

    5 Kauffmann, G., "The Host Galaxies of Active Galactic Nuclei" 346 : 1055-1077, 2003

    6 Athanassoula, E., "The Existence and Shapes of Dust Lanes in Galactic Bars" 259 : 345-364, 1992

    7 Buta. R., "The Distribution of Bar and Spiral Arm Strengths in Disk Galaxies" 130 : 506-523, 2005

    8 van den Wel, A., "The Dependence of Galaxy Morphology and Structure on Environment and Stellar Mass" 675 : 13-16, 2008

    9 Ohta, K., "Surface Photometry of Barred Spiral Galaxies" 357 : 71-90, 1990

    10 Ann, H.B, "Surface Photometry of Barred Galaxies: Global Structure of Barred Galaxies" 20 : 49-62, 1987

    1 형식, "시이펏 은하 NGC 5728의 OASIS 분광 영상" 한국지구과학회 27 (27): 569-578, 2006

    2 Donas, J., "Ultraviolet Observations and Starformation Rate in Galaxies" 180 : 12-26, 1987

    3 Kewley, L.J., "Theoretical Modeling of Starburst Galaxies" 556 : 121-140, 2001

    4 Ho, L.C, "The Influence of Bars on Nuclear Activity" 487 : 591-602, 1997

    5 Kauffmann, G., "The Host Galaxies of Active Galactic Nuclei" 346 : 1055-1077, 2003

    6 Athanassoula, E., "The Existence and Shapes of Dust Lanes in Galactic Bars" 259 : 345-364, 1992

    7 Buta. R., "The Distribution of Bar and Spiral Arm Strengths in Disk Galaxies" 130 : 506-523, 2005

    8 van den Wel, A., "The Dependence of Galaxy Morphology and Structure on Environment and Stellar Mass" 675 : 13-16, 2008

    9 Ohta, K., "Surface Photometry of Barred Spiral Galaxies" 357 : 71-90, 1990

    10 Ann, H.B, "Surface Photometry of Barred Galaxies: Global Structure of Barred Galaxies" 20 : 49-62, 1987

    11 Kennicutt, R.C.Jr, "Star Formation in Galaxies Along the Hubble Sequence" 36 : 189-231, 1998

    12 Hopkins, A.M., "Star Formation Rate Indicators In The Sloan Digital Sky Survey" 599 : 971-991, 2003

    13 Veilleux, S, "Spectral Classification of Emission-line Galaxies" 63 : 295-310, 1987

    14 손동훈, "Seyfert 1 은하 NGC 4151, NGC 5548의 BLR 밀도 변화" 한국지구과학회 25 (25): 495-503, 2004

    15 Sheth, K., "Secular Evolution via Bar-driven gas Inflow: Results from BIMA SONG" 632 : 217-226, 2005

    16 Friedli, D, "Secular Evolution of Isolated Barred Galaxies. II. Coupling between Stars and Interstellar Medium via Star Formation" 301 : 649-665, 1995

    17 Friedli, D, "Secular Evolution of Isolated Barred Galaxies. I-Gravitational Coupling between Stellar Bars and Interstellar Medium" 268 : 65-85, 1993

    18 Ann, H.B, "SPH Simulations of Barred Galaxies: Dynamical Evolution of Gaseous Disk" 33 : 1-17, 2000

    19 HONG-BAEANN, "SECULAR EVOLUTION OF BARRED GALAXIES" 한국천문학회 36 (36): 241-248, 2003

    20 Wada, K, "Rapid Gas Supply to a Nuclear Region by Self-gravitational Instability in a Weak Barred Potential" 258 : 82-94, 1992

    21 Martin, P., "Quantitative Morphology of Bars in Spiral Galaxies" 109 : 2428-2443, 1995

    22 Elmegreen, B.G, "Properties of Barred Spiral Galaxies" 288 : 438-455, 1985

    23 Ann, H.B, "Nuclear Spirals as Signatures of Supermassive Black Holes" 613 : 105-108, 2004

    24 Piner, B.G., "Nuclear Rings and Mass Inflow in Hydrodynamic Simulations of Barred Galaxies" 449 : 508-520, 1995

    25 Simkin, S.M., "Nearby Seyfert Galaxies" 237 : 404-413, 1980

    26 Márquez, I., "Near-infrared Photometry of Isolated Spirals with and without an AGN-II. Photometric Properties of the Host Galaxies" 360 : 431-438, 2000

    27 Eskridge, P.B., "Near-Infrared and Optical Morphology of Spiral Galaxies" 143 : 73-111, 2002

    28 Maciejewski, W., "Gas Inflow in Barred Galaxies - Effects of Secondary Bars" 329 : 502-512, 2002

    29 Dressler, A., "Galaxy Morphology in Rich Clusters - Implications for the Formation and Evolution of Galaxies" 236 : 351-365, 1980

    30 Hasan, H., "Galactic Bars with Central Mass Concentrations-Three-dimensional Dynamics" 409 : 91-109, 1993

    31 Ann, H.B, "Formation of Nuclear Spirals in Barred Galaxies" 620 : 197-209, 2005

    32 Combes, F, "Formation and Properties of Persisting Stellar Bars" 96 : 164-173, 1981

    33 Isobe, T, "Far-infrared Luminosity Functions of Normal Galaxies" 79 : 197-211, 1992

    34 Sheth, K., "Evolution of the Bar Fraction in COSMOS: Quantifying the Assembly of the Hubble Sequence" 675 : 1141-1155, 2008

    35 Park, C., "Environmental Dependence of Properties of Galaxies in the Sloan Digital Sky Survey" 658 : 898-916, 2007

    36 Englmaier, P, "Density Waves inside the Inner Lindblad Resonance: Nuclear Spirals in Disk Galaxies" 528 : 677-686, 2000

    37 Laurikainen, E., "Comparison of Bar Strengths in Active and Non-active Galaxies" 331 : 880-892, 2002

    38 Laurikainen, E, "Comparison of Bar Strengths and Fractions of Bars in Active and Nonactive Galaxies" 607 : 103-124, 2004

    39 Baldwin, J., "Classification Parameters for the Emission-line Spectra of Extragalactic Objects" 93 : 5-19, 1981

    40 Scoville, N., "COSMOS: Hubble Space Telescope Observations" 172 : 38-45, 2007

    41 Barazza, F.D., "Bars in Disk-dominated and Bulge-dominated Galaxies at z ~ 0: New Insights from ~3600 SDSS Galaxies" 675 : 1194-1212, 2008

    42 Regan, M.W, "Bar-driven Mass Inflow: How Bar Characteristics Affect the Inflow" 600 : 595-612, 2004

    43 Laurikainen, E., "Bar Strengths and Nuclear Activity" 249 : 183-186, 2001

    44 Martinet, L, "Bar Strength and Star Formation Activity in Late-type Barred Galaxies" 323 : 363-373, 1997

    45 Norman, C.A., "Bar Dissolution and Bulge Formation: An Example of Secular Dynamical Evolution in Galaxies" 462 : 114-124, 1996

    46 Aguerri, J.A.L., "A strong correlation between bar strength and Global Star Forming Activity in Isolated Barred Galaxies" 351 : 43-46, 1999

    47 Pompea, S.M, "A Test of the Association of Infrared Activity with Bars" 356 : 416-429, 1990

    48 Knapen, J.H., "A Subarcsecond Resolution Near-Infrared Study of Seyfert and Normal Galaxies. II. Morphology" 529 : 93-100, 2000

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