Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

On the magnetic field in the white dwarf Grw + 70 degree 8247

Journal Article · · Astrophysical Journal; (USA)
DOI:https://doi.org/10.1086/184314· OSTI ID:5180221
Greenstein has observed a sharp absorption feature near 1345 {angstrom} in the ultraviolet spectrum of the white dwarf Grw + 70{degree}8247. He interprets this as a component of hydrogen Ly{alpha} in a strong magnetic field, which he estimates to be in the region of 3.5 {times} 10{sup 8} gauss. Using a very accurate multiparameter variational approach, the authors deduce that the maximum Ly{alpha} wavelength obtainable is 1342.6 {angstrom} (or slightly greater if one includes a gravitational redshift as well as a Stark-induced redshift), at which wavelength the magnetic field is 5.6 {times} 10{sup 8} gauss, all other magnetic field values giving rise to smaller wavelengths. In addition, if the authors assume that the observations are uncertain by, say, {plus minus}8 {angstrom}, then the authors deduce that the Ly{alpha} interpretation leads to a white dwarf magnetic field in the range (4.0-7.6) {times} 10{sup 8} gauss. Furthermore, the authors present a (perhaps less likely) alternative interpretation of the 1345 {angstrom} line, viz., that it is a component of H{alpha} at 6.2 {times} 10{sup 8} gauss or a component of H{beta} at 4 {times} 10{sup 8} gauss, or a combination of two other components of H{beta} at 5 {times} 10{sup 8} gauss. 7 refs., 1 tab.
OSTI ID:
5180221
Journal Information:
Astrophysical Journal; (USA), Journal Name: Astrophysical Journal; (USA) Vol. 282; ISSN ASJOA; ISSN 0004-637X
Country of Publication:
United States
Language:
English