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PMAS observations at the Calar Alto 3.5m Teleskop: Measuring the diffuse ionized gas in galaxies

Subject Area Astrophysics and Astronomy
Term from 2019 to 2021
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 438568561
 
The project intends to perform deep PMAS observations of low Halpha surface brightness regions in nearby galaxies to shed light on the nature of the diffuse ionized gas (DIG) component that has often been attributed to Lyman continuum radiation leaking from HII regions. Recent evidence obtained with the MUSE instrument at the VLT is suspiciously pointing to a possible shock excitation origin of the DIG rather than photoionization. We shall utilize the high efficiency of PMAS for low intensity emission to map out regions close to and farther away from luminous HII regions in several nearby galaxies in order to constrain the likely cause for ionization as observable in Ha, Hb, [OI],[OII][OIII],[NII],[SII].
DFG Programme Research Grants
 
 

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