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

New observations of Pa-alpha lines in two quasi-stellar objects

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/167348· OSTI ID:5726964
The importance of internal reddening in QSOs can be assessed by comparison of Pa-alpha line fluxes with Balmer line fluxes. For two QSOs, Pa-alpha lines with a cooled grating spectrometer were observed using a resolving power of 200. In the case of PG 0026 + 129, the Pa-alpha line flux is considerably less than that determined by some earlier, lower resolution measurements. This result suggests that the Pa-alpha lines in other QSOs should also be reobserved with higher resolution. The Pa-alpha/H-alpha line ratios in both QSOs are consistent with standard QSO models without reddening. It is concluded that substantial reddening is unlikely in these objects unless the intrinsic Pa-alpha/H-alpha ratios are lower than those of current models. 35 refs.
Research Organization:
Texas Univ., Austin (USA); CNR, Centro per l'Astronomia Infrarossa, Florence (Italy)
OSTI ID:
5726964
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 339; ISSN ASJOA
Country of Publication:
United States
Language:
English