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Absorption features in the quasar HS 1603 + 3820 II. Distance to the absorber obtained from photoionisation modelling
DOI: 10.1016/j.newast.2013.08.009 Bibcode: 2014NewA...28...70R

Różańska, A.; Hryniewicz, K.; Ebeling, H. +4 more

We present the photoionisation modelling of the intrinsic absorber in the bright quasar HS 1603 + 3820. We constructed the broad-band spectral energy distribution using the optical/UV/X-ray observations from different instruments as inputs for the photoionisation calculations. The spectra from the Keck telescope show extremely high CIV to HI ratio…

2014 New Astronomy
IUE 11
Ultraviolet spectral variations of FK Comae and V 1794 Cygni
DOI: 10.1016/j.newast.2014.02.004 Bibcode: 2014NewA...31...37S

Sanad, M. R.; Bobrowsky, M.

Ultraviolet spectra of FK Comae and V1794 Cygni observed with the Hubble Space Telescope Cosmic Origins Spectrograph (HST COS) and the International Ultraviolet Explorer (IUE) satellites were analyzed for the period 1981-2011. Temporal variations of line fluxes of the O I 1306 Å, C II 1336 Å, C IV 1550 Å, He II 1640 Å and Mg II k & h 2800 Å, p…

2014 New Astronomy
IUE eHST 2
Spectral behavior of 44 (iota) Bootis and VW Cephei in the ultraviolet
DOI: 10.1016/j.newast.2013.12.004 Bibcode: 2014NewA...29...47S

Sanad, M. R.; Bobrowsky, M.

We present ultraviolet spectra of two W UMa-type binary systems, 44 (iota) Boo and VW Cep, with good coverage over their 0.268-day and 0.278-day periods, respectively, using observations obtained with the International Ultraviolet Explorer (IUE) during the period of 1978-1989 and 1978-1992. Three profiles of 44 (iota) Boo and VW Cep showing variat…

2014 New Astronomy
IUE 1
Ultraviolet spectral behavior of IP Peg and DW UMa in high, intermediate and low states from the HST and IUE satellites
DOI: 10.1016/j.newast.2013.09.003 Bibcode: 2014NewA...27...63S

Sanad, M. R.

Ultraviolet spectra of IP Peg and DW UMa observed with Hubble Space Telescope Space Telescope Imaging Spectrograph & Faint Object Spectrograph (HST STIS FOS) and International Ultraviolet Explorer (IUE) satellites were analyzed during the period between 1989-1994 and 1985-2004. Different profiles of two systems showing variations of line fluxe…

2014 New Astronomy
IUE eHST 1