X-RAY SPECTROSCOPY OF 30 DORADUS
30 Doradus represents the most intense starburst in the Local Group of galaxies and powers the spectacular Tarantula Nebula, although the underlying astrophysics remains poorly understood. We propose an XRISM observation to perform the first X-ray spectroscopic study of the starburst region. We will determine the thermal and dynamical states of the massive stellar cluster wind that shapes the nebula, the X-ray contribution from the charge exchange between hot and cool gases, and the presence of the non-thermal X-ray component and hence the cosmic ray acceleration in the region. This study will help us to understand how the starburst feedback works.
TELESCOP= 'XRISM ' / Mission name INSTRUME= 'XTEND ' / Instrument name OBS_ID = '201085010' / Observation identification string OBJECT = '30_DORADUS' / Object name OBSERVER= 'Q. WANG ' / PI name OBS_MODE= 'POINTING' / POINTING or SLEW or ALL RA_OBJ = 84.6713 / [deg] Object Right ascension DEC_OBJ = -69.0963 / [deg] Object Declination RA_PNT = 84.6759079306737 / Pointing RA DEC_PNT = -69.0980997096682 / Pointing DEC RA_NOM = 84.6710711359885 / [deg] Nominal aspect point R.A. DEC_NOM = -69.0961954123845 / [deg] Nominal aspect point Dec. PA_NOM = 8.01350039251359 / [deg] Nominal aspect point roll. TELAPSE = 240373 / Elapsed time DATE-OBS= '2025-07-14T18:04:38' / Start date DATE-END= '2025-07-17T12:50:51' / Stop date ONTIME = 100978.0736 / On-source time EXPOSURE= 100978.0736 / 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 = '2025-07-22T08:18:45' / Date and time this file was created or updated SIB2_VER= 'V04.00 ' / SIB2 version JAXA