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Chromospheric Signatures of Small-scale Flux Emergence as Observed with New Solar Telescope and Hinode Instruments
DOI: 10.1088/0004-637X/722/2/1970 Bibcode: 2010ApJ...722.1970Y

Chae, J.; Goode, P. R.; Abramenko, V. I. +4 more

With the ever-increasing influx of high-resolution images of the solar surface obtained at a multitude of wavelengths, various processes occurring at small spatial scales have become a greater focus of our attention. Complex small-scale magnetic fields have been reported that appear to have enough stored energy to heat the chromosphere. While sign…

2010 The Astrophysical Journal
Hinode 11
Analysis of Spatial Structure of the Spica H II Region
DOI: 10.1088/0004-637X/719/2/1964 Bibcode: 2010ApJ...719.1964P

Park, J. -W.; Min, K. -W.; Edelstein, J. +2 more

Far ultraviolet (FUV) spectral images of the Spica H II region are first presented here for the Si II* λ1533.4 and Al II λ1670.8 lines and then compared with the optical Hα image. The Hα and Si II* images show enhanced emissions in the southern part of the H II region where H I density increases outward. This high density region, which we identify…

2010 The Astrophysical Journal
IUE 11
Multiple Weak Deflections in Galaxy-Galaxy Lensing
DOI: 10.1088/0004-637X/713/1/603 Bibcode: 2010ApJ...713..603B

Brainerd, Tereasa G.

The frequency and effects of multiple weak deflections in galaxy-galaxy lensing are investigated via Monte Carlo simulations. The lenses in the simulations are galaxies with known redshifts and known rest-frame blue luminosities. The frequency of multiple deflections above a given threshold shear value is quantified for discrete source redshifts, …

2010 The Astrophysical Journal
eHST 11
Extinction and Distance to Anomalous X-ray Pulsars from X-ray Scattering Halos
DOI: 10.1088/0004-637X/710/1/797 Bibcode: 2010ApJ...710..797R

van Kerkwijk, M. H.; Rivera-Ingraham, A.

We analyze the X-ray scattering halos around three Galactic Anomalous X-ray Pulsars in order to constrain the distance and the optical extinction of each source. We obtain surface brightness distributions from EPIC-pn data obtained with XMM-Newton, compare the profiles of different sources, and fit them with a model based on the standard theory of…

2010 The Astrophysical Journal
XMM-Newton 11
The Role of Magnetic Topology in the Heating of Active Region Coronal Loops
DOI: 10.1088/0004-637X/723/2/1493 Bibcode: 2010ApJ...723.1493L

Reeves, Katharine K.; Golub, L.; Leka, K. D. +4 more

We investigate the evolution of coronal loop emission in the context of the coronal magnetic field topology. New modeling techniques allow us to investigate the magnetic field structure and energy release in active regions (ARs). Using these models and high-resolution multi-wavelength coronal observations from the Transition Region and Coronal Exp…

2010 The Astrophysical Journal
Hinode SOHO 11
Cosmic-ray Spallation in Radio-quiet Active Galactic Nuclei: A Case Study of NGC 4051
DOI: 10.1088/0004-637X/709/2/1230 Bibcode: 2010ApJ...709.1230T

Turner, T. J.; Miller, L.

We investigate conditions for and consequences of spallation in radio-quiet Seyfert galaxies. The work is motivated by the recent discovery of significant line emission at 5.44 keV in Suzaku data from NGC 4051. The energy of the new line suggests an identification as Cr I Kα emission; however, the line is much stronger than would be expected from …

2010 The Astrophysical Journal
Suzaku 11
Fine Magnetic Features and Chirality in Solar Active Region NOAA 10930
DOI: 10.1088/0004-637X/716/2/1493 Bibcode: 2010ApJ...716.1493Z

Zhang, Hongqi

In this paper, we present fine magnetic features near the magnetic inversion line in the solar active region NOAA 10930. The high-resolution vector magnetograms obtained by Hinode allow detailed analyses around magnetic fibrils in the active region. The analyses are based on the fact that the electric current density can be divided into two compon…

2010 The Astrophysical Journal
Hinode 11
XMM-Newton Observations of the Seyfert 2 Galaxy NGC 7590: The Nature of X-ray Absorption
DOI: 10.1088/0004-637X/722/1/96 Bibcode: 2010ApJ...722...96S

Shu, X. W.; Wang, J. X.; Liu, T.

We present the analysis of three XMM-Newton observations of the Seyfert 2 galaxy NGC 7590. The source was found to have no X-ray absorption in the low spatial resolution ASCA data. The XMM-Newton observations provide a factor of ~10 better spatial resolution than previous ASCA data. We find that the X-ray emission of NGC 7590 is dominated by an of…

2010 The Astrophysical Journal
XMM-Newton 11
The Opacity of Galactic Disks at z ~ 0.7
DOI: 10.1088/2041-8205/714/1/L113 Bibcode: 2010ApJ...714L.113S

Kneib, J. -P.; Ilbert, O.; Taniguchi, Y. +13 more

We compare the surface brightness-inclination relation for a sample of COSMOS pure disk galaxies at z ~ 0.7 with an artificially redshifted sample of Sloan Digital Sky Survey (SDSS) disks well matched to the COSMOS sample in terms of rest-frame photometry and morphology, as well as their selection and analysis. The offset between the average surfa…

2010 The Astrophysical Journal
eHST 10
Ignition Column Depths of Helium-rich Thermonuclear Bursts from 4U 1728-34
DOI: 10.1088/0004-637X/718/2/947 Bibcode: 2010ApJ...718..947M

Galloway, Duncan K.; Misanovic, Zdenka; Cooper, Randall L.

We analyzed thermonuclear (type I) X-ray bursts observed from the low-mass X-ray binary 4U 1728-34 by RXTE, Chandra, and INTEGRAL. We compared the variation in burst energy and recurrence times as a function of accretion rate with the predictions of a numerical ignition model including a treatment of the heating and cooling in the crust. We found …

2010 The Astrophysical Journal
INTEGRAL 10