The SAMI Galaxy Survey: the low-redshift stellar mass Tully–Fisher relation

The SAMI Galaxy Survey: the low-redshift stellar mass Tully–Fisher relation

Abstract We investigate the Tully–Fisher relation (TFR) for a morphologically and kinematically diverse sample of galaxies from the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey using two-dimensional spatially resolved H α velocity maps and find a well-defined relation acr...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2017-12, Vol.472 (2), p.1809-1824
Hauptverfasser: Bloom, J. V., Croom, S. M., Bryant, J. J., Callingham, J. R., Schaefer, A. L., Cortese, L., Hopkins, A. M., D'Eugenio, F., Scott, N., Glazebrook, K., Tonini, C., McElroy, R. E., Clark, H. A., Catinella, B., Allen, J. T., Bland-Hawthorn, J., Goodwin, M., Green, A. W., Konstantopoulos, I. S., Lawrence, J., Lorente, N., Medling, A. M., Owers, M. S., Richards, S. N., Sharp, R.
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Sprache:eng
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Zusammenfassung:Abstract We investigate the Tully–Fisher relation (TFR) for a morphologically and kinematically diverse sample of galaxies from the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey using two-dimensional spatially resolved H α velocity maps and find a well-defined relation across the stellar mass range of 8.0 
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stx1701