Abstract
view Abstract Citations (57) References (53) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Two New Extremely Iron-rich Hot DA White Dwarfs and the Nature of the EUV Opacity Holberg, J. B. ; Barstow, M. A. ; Buckley, D. A. H. ; Chen, A. ; Dreizler, S. ; Marsh, M. C. ; O'Donoghue, D. ; Sion, E. M. ; Tweedy, R. W. ; Vauclair, G. ; Werner, K. Abstract We have obtained IUE echelle spectra of two bright extreme ultraviolet (EUV) sources discovered by the ROSAT wide field camera all-sky survey. These stars, RE 2214-492 and RE 0623-377, are previously uncataloged hot DA white dwarfs with respective apparent visual magnitudes of 11.71 and 12.09 and exhibit short-wavelength EUV cutoffs steeper than most other DAs. The IUE echelle spectra are rich in absorption lines due to a large number of Fe V and Fe VI features, in addition to the highly ionized C, N, O ions frequently seen in other hot DA white dwarfs. No He is observed in either star. Comparison of RE 2214-492 and RE 0623-377 with two well-studied hot DA white dwarfs, G191 B2B and Feige 24, indicates that these new stars are both significantly hotter and more metal-rich than G191 B2B and Feige 24. From optical and UV line profiles we find Teff = 63,500 K and 60,300 K for RE 2214-492 and RE 0623-377, respectively. From modeling of Fe V features in the echelle spectra we find corresponding Fe abundances of log [N(Fe)/ n(H)] = -4.25±0.25. The association of steep EUV cutoffs in these stars, and in G191 B2B and Feige 24, with the observed presence of Fe suggests that iron-group elements along with other heavy elements are responsible for much of the EUV opacity observed by ROSA T in the hottest DA stars. Publication: The Astrophysical Journal Pub Date: October 1993 DOI: 10.1086/173278 Bibcode: 1993ApJ...416..806H Keywords: STARS: INDIVIDUAL ALPHANUMERIC: RE 0623-377; STARS: INDIVIDUAL ALPHANUMERIC: RE 2214-492; STARS: WHITE DWARFS; STARS: ABUNDANCES; ULTRAVIOLET: STARS full text sources ADS | data products SIMBAD (7) MAST (1) INES (1)
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