MASS MEASUREMENT OF THE WHITE DWARF IN EX HYA WITH HIGH RESOLUTION X-RAY SPECTROSCOPY
The mass of white dwarfs (WDs) within binary systems is a crucial parameter for understanding their evolution into type-Ia supernovae. Among WD binary systems, we focus on the X-ray luminous object, the intermediate polars (IPs) for XRISM observations. The measurement of gravitational redshifts and the bulk Doppler shifts of atomic lines have proven to be robust tools for mass determination, as demonstrated by Hayashi et al.(2023) with Chandra HETG data. We propose a 75 ksec XRISM observation of the IP system EX Hya, to which we already applied the method for lighter elements, to ascertain the WD mass with 10% accuracy with Fe-K lines.
TELESCOP= 'XRISM ' / Mission name INSTRUME= 'XTEND ' / Instrument name OBS_ID = '201058010' / Observation identification string OBJECT = 'EX_HYA ' / Object name OBSERVER= 'TAICHI ICHIKAWA' / PI name OBS_MODE= 'POINTING' / POINTING or SLEW or ALL RA_OBJ = 193.1009 / [deg] Object Right ascension DEC_OBJ = -29.2489 / [deg] Object Declination RA_PNT = 193.103979673339 / Pointing RA DEC_PNT = -29.2477929085498 / Pointing DEC RA_NOM = 193.101334499172 / [deg] Nominal aspect point R.A. DEC_NOM = -29.2489232954401 / [deg] Nominal aspect point Dec. PA_NOM = 294.100314904517 / [deg] Nominal aspect point roll. TELAPSE = 163248 / Elapsed time DATE-OBS= '2025-07-12T19:26:45' / Start date DATE-END= '2025-07-14T16:47:33' / Stop date ONTIME = 76612.566095 / On-source time EXPOSURE= 76612.566095 / Exposure time PROCVER = '03.02.014.010' / Processing script version MKFFF = 'ISAS/JAXA' / Origin of First FITS file ORIGIN = 'GSFC/NASA' / Origin of Processed FITS file SOFTVER = 'Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002' / Version of HEADAS used CALDBVER= 'gen20241115_xtd20241115_rsl20241115' / Version of CALDB used DATE = '2025-07-19T02:24:58' / Date and time this file was created or updated SIB2_VER= 'V04.00 ' / SIB2 version JAXA