| Issue |
A&A
Volume 683, March 2024
|
|
|---|---|---|
| Article Number | C3 | |
| Number of page(s) | 1 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/202449493e | |
| Published online | 13 March 2024 | |
Molecular gas in super spiral galaxies (Corrigendum)
1
Departamento de Física Teórica y del Cosmos, Universidad de Granada, 18071 Granada, Spain
e-mail: ute@ugr.es
2
Instituto Carlos I de Física Téorica y Computacional, Facultad de Ciencias, 18071 Granada, Spain
3
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
4
Caltech/IPAC, 1200 E. California Blvd., Pasadena, CA 91125, USA
5
Department of Astronomy, University of Cape Town, Private Bag X3, Rondebosch 7701, South Africa
6
Department of Physics, University of Bath, Claverton Down, Bath BA2 7AY, UK
Key words: galaxies: evolution / galaxies: ISM / galaxies: spiral / ISM: molecules / errata / addenda
We have noticed an error in Eq. (9) of our original paper. Furthermore, in the paragraph below, we provide an explanation of how LW3, dust and LW4, dust were calculated, which was not described correctly in our paper.
The correct form of Eq. (9), which was correctly applied in the paper, is the following:
![$$ \begin{aligned} \mathrm{SFR}_{\rm W3,C17} [M_\odot \,\mathrm{yr}^{-1}] = (L_{\rm W3,dust})^{0.889} 10^{-37.81}, \end{aligned} $$](/articles/aa/full_html/2024/03/aa49493e-24/aa49493e-24-eq1.gif)
where LNUV is the luminosity of the Galaxy Evolution Explorer (GALEX) near-ultraviolet (NUV) band and LW3, dust, LW4, dust are the luminosities from the dust contribution to the Wide-field Infrared Survey Explorer (WISE) W3 and W4 bands. Thelatter was obtained from the total luminosities in these bands after subtracting the stellar continuum based on the W1 luminosity, LW1, calculated following Jarrett et al. (2017) as cited in Cluver et al. (2017), as LW3, stellar = 0.158 × LW1 and LW4, stelllar = 0.059 × LW1 (very similar to the coefficients of Janowiecki; LW3, stellar, J17 = 0.201 × LW1, and LW4, stellar, J17 = 0.044 × LW1). All luminosities are defined as νLν and are in units oferg s−1.
References
- Cluver, M. E., Jarrett, T. H., Dale, D. A., et al. 2017, ApJ, 850, 68 [Google Scholar]
- Jarrett, T. H., Cluver, M. E., Magoulas, C., et al. 2017, ApJ, 836, 182 [Google Scholar]
© The Authors 2024
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