Searching the Non‐Accreting White Dwarf Population in eROSITA Data
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DOI: 10.1002/asna.20240139
Abstract: eROSITA is the soft X‐ray instrument aboard the Spectrum Roentgen Gamma (SRG) satellite that is most sensitive in the energy range between 0.2 and 2.3 keV. Between December 2019 and December 2021, eROSITA completed four all‐sky… read more here.
Keywords: accreting white; non accreting; white dwarf; searching non ... See more keywords