| Parameter . | Value . | Reference . |
|---|---|---|
| Right Ascension (J2000.0) | |$14^\mathrm{h}53^\mathrm{m}57\rm{.\!\!^{\rm {\mathrm{s}}}}57$| | 1 |
| Declination (J2000.0) | +03○32′40|${_{.}^{\prime\prime}}$|1 | 1 |
| Adopted distance | 28.9 Mpc | 2 |
| Angular scale | 7.14 arcsec kpc−1 | 2 |
| Diameter of the stellar disc (D25) | |$4.17~{\rm arcmin} = 35.0\, \mathrm{kpc}$| | 3 |
| Diameter of the star forming (H α) disc | |$3.58~{\rm arcmin} = 30.1\, \mathrm{kpc}$| | 4 |
| Diameter of the radio continuum disc | |$4.7~{\rm arcmin} = 39.5\, \mathrm{kpc}$| | 4 |
| Adopted (H α+IR) star formation rate (SFR)a | |$7.56\pm 0.65\, \mathrm{M_{\odot }\, yr^{-1}}$| | 5 |
| SFR surface density | |$(9.41\pm 0.81)\times 10^{-3}\, \mathrm{M_{\odot }\, yr^{-1}\, kpc^{-2}}$| | 5 |
| Alternative (1.4 GHz) SFRa | |$22.9\, \mathrm{M_{\odot }\, yr^{-1}}$| | 4 |
| Inclination | 85|${_{.}^{\circ}}$|8 | 1 |
| Position angle | 145|${_{.}^{\circ}}$|7 | 1 |
| Maximum midplane |$v$|rot | |$198\, \mathrm{km\, s^{-1}}$| | 1 |
| Vertical rotation gradient (d|$v$|rot/d|$z$|) | |$1\, \mathrm{km\, s^{-1}\, arcsec^{-1}}=7\, \mathrm{km\, s^{-1}\, kpc^{-1}}$| | 6 |
| Parameter . | Value . | Reference . |
|---|---|---|
| Right Ascension (J2000.0) | |$14^\mathrm{h}53^\mathrm{m}57\rm{.\!\!^{\rm {\mathrm{s}}}}57$| | 1 |
| Declination (J2000.0) | +03○32′40|${_{.}^{\prime\prime}}$|1 | 1 |
| Adopted distance | 28.9 Mpc | 2 |
| Angular scale | 7.14 arcsec kpc−1 | 2 |
| Diameter of the stellar disc (D25) | |$4.17~{\rm arcmin} = 35.0\, \mathrm{kpc}$| | 3 |
| Diameter of the star forming (H α) disc | |$3.58~{\rm arcmin} = 30.1\, \mathrm{kpc}$| | 4 |
| Diameter of the radio continuum disc | |$4.7~{\rm arcmin} = 39.5\, \mathrm{kpc}$| | 4 |
| Adopted (H α+IR) star formation rate (SFR)a | |$7.56\pm 0.65\, \mathrm{M_{\odot }\, yr^{-1}}$| | 5 |
| SFR surface density | |$(9.41\pm 0.81)\times 10^{-3}\, \mathrm{M_{\odot }\, yr^{-1}\, kpc^{-2}}$| | 5 |
| Alternative (1.4 GHz) SFRa | |$22.9\, \mathrm{M_{\odot }\, yr^{-1}}$| | 4 |
| Inclination | 85|${_{.}^{\circ}}$|8 | 1 |
| Position angle | 145|${_{.}^{\circ}}$|7 | 1 |
| Maximum midplane |$v$|rot | |$198\, \mathrm{km\, s^{-1}}$| | 1 |
| Vertical rotation gradient (d|$v$|rot/d|$z$|) | |$1\, \mathrm{km\, s^{-1}\, arcsec^{-1}}=7\, \mathrm{km\, s^{-1}\, kpc^{-1}}$| | 6 |
Notes. References: (1) Irwin (1994); (2) Irwin et al. (2012); (3) de Vaucouleurs et al. (1991); (4) this work; (5) Vargas et al. (2019); (6) Heald et al. (2006).
aFrom the Murphy et al. (2011) calibrations, assuming a Kroupa IMF between 0.1–|$100\, \mathrm{M_\odot }$|.
| Parameter . | Value . | Reference . |
|---|---|---|
| Right Ascension (J2000.0) | |$14^\mathrm{h}53^\mathrm{m}57\rm{.\!\!^{\rm {\mathrm{s}}}}57$| | 1 |
| Declination (J2000.0) | +03○32′40|${_{.}^{\prime\prime}}$|1 | 1 |
| Adopted distance | 28.9 Mpc | 2 |
| Angular scale | 7.14 arcsec kpc−1 | 2 |
| Diameter of the stellar disc (D25) | |$4.17~{\rm arcmin} = 35.0\, \mathrm{kpc}$| | 3 |
| Diameter of the star forming (H α) disc | |$3.58~{\rm arcmin} = 30.1\, \mathrm{kpc}$| | 4 |
| Diameter of the radio continuum disc | |$4.7~{\rm arcmin} = 39.5\, \mathrm{kpc}$| | 4 |
| Adopted (H α+IR) star formation rate (SFR)a | |$7.56\pm 0.65\, \mathrm{M_{\odot }\, yr^{-1}}$| | 5 |
| SFR surface density | |$(9.41\pm 0.81)\times 10^{-3}\, \mathrm{M_{\odot }\, yr^{-1}\, kpc^{-2}}$| | 5 |
| Alternative (1.4 GHz) SFRa | |$22.9\, \mathrm{M_{\odot }\, yr^{-1}}$| | 4 |
| Inclination | 85|${_{.}^{\circ}}$|8 | 1 |
| Position angle | 145|${_{.}^{\circ}}$|7 | 1 |
| Maximum midplane |$v$|rot | |$198\, \mathrm{km\, s^{-1}}$| | 1 |
| Vertical rotation gradient (d|$v$|rot/d|$z$|) | |$1\, \mathrm{km\, s^{-1}\, arcsec^{-1}}=7\, \mathrm{km\, s^{-1}\, kpc^{-1}}$| | 6 |
| Parameter . | Value . | Reference . |
|---|---|---|
| Right Ascension (J2000.0) | |$14^\mathrm{h}53^\mathrm{m}57\rm{.\!\!^{\rm {\mathrm{s}}}}57$| | 1 |
| Declination (J2000.0) | +03○32′40|${_{.}^{\prime\prime}}$|1 | 1 |
| Adopted distance | 28.9 Mpc | 2 |
| Angular scale | 7.14 arcsec kpc−1 | 2 |
| Diameter of the stellar disc (D25) | |$4.17~{\rm arcmin} = 35.0\, \mathrm{kpc}$| | 3 |
| Diameter of the star forming (H α) disc | |$3.58~{\rm arcmin} = 30.1\, \mathrm{kpc}$| | 4 |
| Diameter of the radio continuum disc | |$4.7~{\rm arcmin} = 39.5\, \mathrm{kpc}$| | 4 |
| Adopted (H α+IR) star formation rate (SFR)a | |$7.56\pm 0.65\, \mathrm{M_{\odot }\, yr^{-1}}$| | 5 |
| SFR surface density | |$(9.41\pm 0.81)\times 10^{-3}\, \mathrm{M_{\odot }\, yr^{-1}\, kpc^{-2}}$| | 5 |
| Alternative (1.4 GHz) SFRa | |$22.9\, \mathrm{M_{\odot }\, yr^{-1}}$| | 4 |
| Inclination | 85|${_{.}^{\circ}}$|8 | 1 |
| Position angle | 145|${_{.}^{\circ}}$|7 | 1 |
| Maximum midplane |$v$|rot | |$198\, \mathrm{km\, s^{-1}}$| | 1 |
| Vertical rotation gradient (d|$v$|rot/d|$z$|) | |$1\, \mathrm{km\, s^{-1}\, arcsec^{-1}}=7\, \mathrm{km\, s^{-1}\, kpc^{-1}}$| | 6 |
Notes. References: (1) Irwin (1994); (2) Irwin et al. (2012); (3) de Vaucouleurs et al. (1991); (4) this work; (5) Vargas et al. (2019); (6) Heald et al. (2006).
aFrom the Murphy et al. (2011) calibrations, assuming a Kroupa IMF between 0.1–|$100\, \mathrm{M_\odot }$|.
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