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MV Lyrae in Low, Intermediate, and High States
DOI: 10.1086/429143 Bibcode: 2005ApJ...624..923L

Szkody, Paula; Sion, Edward M.; Hoard, D. W. +4 more

Archival IUE spectra of the VY Sculptoris system MV Lyrae, taken during an intermediate state, can be best fit by an isothermal accretion disk extending half-way to the tidal cutoff radius. In contrast, a recent HST spectrum, while MV Lyr was in a high state, can be best fit with a standard T(R) profile for an accretion disk extending from an inne…

2005 The Astrophysical Journal
IUE eHST 42
Chandra Observations of NGC 4261 (3C 270): Revealing the Jet and Hidden Active Galactic Nucleus in a Type 2 LINER
DOI: 10.1086/430044 Bibcode: 2005ApJ...627..711Z

Zezas, A.; Fabbiano, G.; Birkinshaw, M. +2 more

We present results from a Chandra ACIS-S observation of the type 2 low-ionization nuclear emission-line region (LINER) radio galaxy NGC 4261 (3C 270). The X-ray data show that this galaxy hosts a heavily obscured (NH~8×1022 cm-2) active galactic nucleus (AGN) with an intrinsic luminosity of 2.4×1041 ergs…

2005 The Astrophysical Journal
eHST 42
Do Young Galaxies Exist in the Local Universe? Red Giant Branch Detection in the Metal-poor Dwarf Galaxy SBS 1415+437
DOI: 10.1086/497112 Bibcode: 2005ApJ...631L..45A

Leitherer, C.; Tosi, M.; van der Marel, R. P. +3 more

We present results from an HST/ACS imaging study of the metal-poor blue compact dwarf galaxy SBS 1415+437. It has been argued previously that this is a very young galaxy that started to form stars only <~100 Myr ago. However, we find that the optical color-magnitude diagram prominently reveals asymptotic giant branch and red giant branch (RGB) …

2005 The Astrophysical Journal
eHST 42
New Elemental Abundances for V1974 Cygni
DOI: 10.1086/428895 Bibcode: 2005ApJ...624..914V

Shore, S. N.; Starrfield, S.; Wagner, R. M. +2 more

We present a new analysis of existing optical and ultraviolet spectra of the ONeMg nova V1974 Cygni 1992. Using these data and the photoionization code Cloudy, we have determined the physical parameters and elemental abundances for this nova. Many of the previous studies of this nova have made use of incorrect analyses, and hence a new study was r…

2005 The Astrophysical Journal
IUE eHST 42
Constraining the Distribution of L and T Dwarfs in the Galaxy
DOI: 10.1086/497368 Bibcode: 2005ApJ...631L.159R

Hathi, N. P.; Ryan, R. E., Jr.; Windhorst, R. A. +1 more

We estimate the thin-disk scale height of the Galactic population of L and T dwarfs based on star counts from 15 deep parallel fields from the Hubble Space Telescope. From these observations, we have identified 28 candidate L and T dwarfs based on their i'-z' color and morphology. By comparing these star counts with a simple Galactic model, we est…

2005 The Astrophysical Journal
eHST 42
XTE J1550-564: INTEGRAL Observations of a Failed Outburst
DOI: 10.1086/429815 Bibcode: 2005ApJ...625..923S

Shrader, C. R.; Sturner, S. J.

The well-known black hole X-ray binary transient XTE J1550-564 underwent an outburst during the spring of 2003, which was substantially underluminous in comparison to previous periods of peak activity in that source. In addition, our analysis shows that it apparently remained in the hard spectral state over the duration of that outburst. This is a…

2005 The Astrophysical Journal
INTEGRAL 41
FUSE Determination of a Low Deuterium Abundance along an Extended Sight Line in the Galactic Disk
DOI: 10.1086/497574 Bibcode: 2005ApJ...635.1136H

Moos, H. W.; Chayer, P.; Dupuis, J. +5 more

We present a study of the deuterium abundance along the extended sight line toward HD 90087 with the Far Ultraviolet Spectroscopic Explorer (FUSE). HD 90087 is a O9.5 III star located in the Galactic disk at a distance of ~2.7 kpc away from the Sun. Both in terms of distance and column densities, HD 90087 has the longest and densest sight line obs…

2005 The Astrophysical Journal
IUE 41
Sculpting a Pre-planetary Nebula with a Precessing Jet: IRAS 16342-3814
DOI: 10.1086/429586 Bibcode: 2005ApJ...622L..53S

Sahai, R.; Sánchez Contreras, C.; Le Mignant, D. +2 more

We have imaged the bipolar pre-planetary nebula IRAS 16342-3814 with the Keck adaptive optics (AO) system in four near-infrared bands in the 1.6-4.7 µm range. The lobes, which showed smoothly varying brightness distributions in previous optical images taken with the Hubble Space Telescope, have a limb-brightened appearance in the AO images, …

2005 The Astrophysical Journal
eHST 41
Isothermal Bias of the ``Filter Ratio'' Method for Observations of Multithermal Plasma
DOI: 10.1086/499125 Bibcode: 2005ApJ...635L.101W

Schmelz, J. T.; DeLuca, E. E.; Weber, M. A. +1 more

An early result from the Transition Region and Coronal Explorer (TRACE) was that the EUV filter ratios for many narrow coronal loops (widths of a few arcseconds) were found to cluster within the small range 0.50-1.70, as functions of position along loop length. The most common interpretation is that the temperature along the loop is in fact nearly…

2005 The Astrophysical Journal
SOHO 41
Abundances and Depletions of Interstellar Oxygen
DOI: 10.1086/426781 Bibcode: 2005ApJ...619..891J

Snow, Theodore P.; Rachford, Brian L.; Jensen, Adam G.

We report on the abundance of interstellar neutral oxygen (O I) for 26 sight lines, using data from the Far Ultraviolet Spectroscopic Explorer, the International Spectroscopic Explorer, and the Hubble Space Telescope. O I column densities are derived by measuring the equivalent widths of several ultraviolet absorption lines and subsequently fittin…

2005 The Astrophysical Journal
IUE eHST 41