High Resolution EUV Spectroscopy of Feige 24 Martin Barstow Department of Physics & Astronomy www.le.ac.uk.

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Presentation transcript:

High Resolution EUV Spectroscopy of Feige 24 Martin Barstow Department of Physics & Astronomy

Introduction Background – EUVE results J-PEX instrument Science goals of Feige 24 Observation Results of 2008 J-PEX flight Future prospects

Science background Limitations of ~ Å resolution spectroscopy with EUVE Detection of photospheric, interstellar or circumstellar He II The composition and structure of white dwarf atmospheres

Helium in EUV Spectra HZ 43

-B2B Helium in EUV Spectra Helium I Helium II

Interstellar Helium

EUVE - Homogeneous Fe Mixture G191-B2B

EUVE - Stratified Fe G191-B2B requires ISM He II /He~75%

The J-PEX Spectrometer R~6000 (δλ=0.04Å) Ion etched, blazed grating. MoSi multilayers for high reflection Spherical figure, 2.2m focal length

Nitrogen IV Oxygen IV Helium II J-PEX

10σ 5σ5σ 3σ3σ 1σ1σ 2σ2σ

Pre-CV Feige 24 Period = 4.23d T eff (wd) = 62,000K K wd ~ 50 km s -1 γ total ~ 70 km s -1 v ISM ~ -10 km s -1

Feige 24 science goals Search for evidence of photospheric He –Measure H layer mass Measure the He II interstellar column density –Derive ionization fraction Search for circumstellar material Exposure time shorter than planned –Reduced signal to noise

Black Brant White Sands Missile Range October 21 st 2008

b) a) c) Feige 24; DA+dM a)H-layer mass = M  b)H-layer mass = M  c)H-layer mass = M  N He II = 3.9x10 17 cm -2 N He I = 1.6x10 17 cm -2 He II /He = 0.72

Conclusion Achieved primary science goal –Limits on H layer mass –Value of He II interstellar component (He II /He = 0.72) Need longer exposure times and more observations –Translate J-PEX onto a satellite platform

b) a) c) Feige 24; DA+dM a)H-layer mass = M  b)H-layer mass = M  c)H-layer mass = M  N He II = 3.9x10 17 cm -2 N He I = 1.6x10 17 cm -2 He II /He = 0.72

Feige 24 simulation, exposure = 4000s

SAGE

EUV spectroscopy flight options In the USA –Low-cost conversion of rocket payloads to ~6 month duration orbital instruments –Response to forthcoming Explorer call In Europe –Submission to latest M-class mission call We need your support... please contact me for involvement