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• W2024304937 endingPage "569" @default.
• W2024304937 startingPage "554" @default.
• W2024304937 abstract "Super star clusters (SSCs) are typically found in interacting galaxies and trace an extreme form of star-formation. We present a K-band study of SSC candidates in a sample of local luminous infrared galaxies (LIRGs) using two adaptive optics instruments (VLT/NACO and Gemini/ALTAIR/NIRI). In addition to facilitating SSC detections in obscured environments, this work introduces SSC studies in hosts with higher star-formation rates (SFRs) than most previous studies. We find that the luminosity functions (LFs) of the clusters are reasonably well-fitted by a single power-law with the values of the index alpha ranging between 1.5 to 2.4 with an average value of alpha ~ 1.9. This value appears to be less steep than the average alpha ~ 2.2 in normal spiral galaxies. Due to the host galaxy distances involved (median $D_L$ ~ 70 Mpc) blending effects have to be taken into account, and are investigated using Monte Carlo simulations of blending effects for LFs and a photometric SSC analysis of the well-studied Antennae system which is artificially redshifted to distances of our sample. While blending tends to flatten LFs our analyses show that Delta alpha is less than ~ 0.1 in our sample. The simulations also show that in the luminosity range, $M_K < -13$, considered in this work the extracted SSC luminosities are generally dominated by a single dominant star cluster rather than several knots of SF. We present resolution- and distance-dependent SSC surface density confusion limits and show how blending rates and aperture sizes affect the LFs. The smallest possible apertures should be used in crowded regions." @default.
• W2024304937 created "2016-06-24" @default.
• W2024304937 creator A5000721632 @default.
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• W2024304937 date "2013-03-07" @default.
• W2024304937 modified "2023-09-23" @default.
• W2024304937 title "The K-band luminosity functions of super star clusters in luminous infrared galaxies, their slopes and the effects of blending" @default.
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• W2024304937 doi "https://doi.org/10.1093/mnras/stt185" @default.
• W2024304937 hasPublicationYear "2013" @default.
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