“STARBIRDS”的版本间差异
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（创建页面，内容为“*Eleven galaxies are from the STARBurst IRRegular Dwarf Sur- vey (STARBIRDS McQuinn et al. 2015b) *All galaxies have previously derived star formation histories from…”） |
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*Preliminary ionized gas kinematics are available from an on-going IFU spectroscopic observing campaign (L. van Zee et al. in preparation). |
*Preliminary ionized gas kinematics are available from an on-going IFU spectroscopic observing campaign (L. van Zee et al. in preparation). |
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*Three galaxies have Chandra X-ray imaging of the hot phase winds (McQuinn et al. 2018) |
*Three galaxies have Chandra X-ray imaging of the hot phase winds (McQuinn et al. 2018) |
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*KPNO Ha images |
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2019年10月16日 (三) 02:13的最新版本
- Eleven galaxies are from the STARBurst IRRegular Dwarf Sur- vey (STARBIRDS McQuinn et al. 2015b)
- All galaxies have previously derived star formation histories from HST observations of their resolved stellar populations (McQuinn et al. 2009, 2010a, 2015b) and measurements of the spatial distribution of recent star formation (McQuinn et al. 2012).
- All galaxies have existing Hi observations to compare with the ionized gas distributions
- Preliminary ionized gas kinematics are available from an on-going IFU spectroscopic observing campaign (L. van Zee et al. in preparation).
- Three galaxies have Chandra X-ray imaging of the hot phase winds (McQuinn et al. 2018)
- KPNO Ha images