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Soft X-Ray and Ultraviolet Emission Relations in Optically Selected AGN Samples
DOI: 10.1086/431247 Bibcode: 2005AJ....130..387S

Brandt, W. N.; Schneider, Donald P.; Vignali, Cristian +2 more

Using a sample of 228 optically selected active galactic nuclei (AGNs) in the 0.01-6.3 redshift range with a high fraction of X-ray detections (81%-86%), we study the relation between rest-frame UV and soft X-ray emission and its evolution with cosmic time. The majority of the AGNs in our sample (155 objects) have been selected from the Sloan Digi…

2005 The Astronomical Journal
IUE XMM-Newton 248
An Analysis of the Shapes of Ultraviolet Extinction Curves. IV. Extinction without Standards
DOI: 10.1086/431900 Bibcode: 2005AJ....130.1127F

Fitzpatrick, E. L.; Massa, D.

In this paper we present a new method for deriving UV through IR extinction curves, based on the use of stellar atmosphere models to provide estimates of the intrinsic (i.e., unreddened) stellar spectral energy distributions (SEDs), rather than unreddened (or lightly reddened) standard stars. We show that this ``extinction without standards'' tech…

2005 The Astronomical Journal
IUE 73
Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry
DOI: 10.1086/427855 Bibcode: 2005AJ....129.1642F

Fitzpatrick, E. L.; Massa, D.

We present a new calibration of optical (UBV, Strömgren uvbyβ, and Geneva) and near-IR (Johnson RIJHK and Two Micron All Sky Survey) photometry for B and early A stars derived from Kurucz ATLAS9 model atmospheres. Our sample of stars consists of 45 normal nearby B and early A stars that have high-quality, low-resolution IUE spectra and accurate Hi…

2005 The Astronomical Journal
Hipparcos IUE 45
On the Ga II and Ga III Resonance Lines and the Implication for Chemical Stratification in HgMn Stars
DOI: 10.1086/491703 Bibcode: 2005AJ....130.2312N

Nielsen, K. E.; Leckrone, D. S.; Wahlgren, G. M. +2 more

The gallium abundance in HgMn stars has been reported to be different for analyses conducted from spectral lines in the optical versus those from the ultraviolet. We pursue this ultraviolet-optical discrepancy from a line-blending perspective by investigating the Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS) spectrum of …

2005 The Astronomical Journal
IUE eHST 13
Escape of Lyα Emission in the Starburst Galaxy Markarian 357: a Wind's Far Side
DOI: 10.1086/428371 Bibcode: 2005AJ....129.1863K

Keel, William C.

Hubble Space Telescope imaging and slitless spectroscopy are used to examine where the strong Lyα emission escapes from the interstellar medium in the starburst galaxy Mrk 357. An Hα image shows that the ionized gas is mostly in a global wind, rather than associated with the individual star-forming regions seen in the optical and UV continuum. The…

2005 The Astronomical Journal
IUE eHST 13
Spin-resolved Far-Ultraviolet Observations of the Magnetic White Dwarf in YY Draconis
DOI: 10.1086/430749 Bibcode: 2005AJ....130..214H

Szkody, Paula; Sion, Edward M.; Hoard, D. W. +1 more

We observed the intermediate polar YY Draconis with the Far Ultraviolet Spectroscopic Explorer (FUSE), yielding an average far-UV spectrum, as well as spectra and spectrophotometric light curves resolved on the spin phase of the white dwarf in this system. We utilized the BINSYN software suite to calculate model spectra based on a simple system mo…

2005 The Astronomical Journal
IUE eHST 7