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Color and Stellar Population Gradients in Passively Evolving Galaxies at z ~ 2 from HST/WFC3 Deep Imaging in the Hubble Ultra Deep Field
DOI: 10.1088/0004-637X/735/1/18 Bibcode: 2011ApJ...735...18G

Papovich, Casey; Dickinson, Mark; Ferguson, Henry C. +10 more

We report the detection of color gradients in six massive (stellar mass (M star) > 1010 M ) and passively evolving (specific star formation rate <10-11 yr-1) galaxies at redshift 1.3 < z < 2.5 identified in the Hubble Ultra Deep Field using ultra-deep Hubble Space Telescope (HST) …

2011 The Astrophysical Journal
eHST 77
The First Observations of Low-redshift Damped Lyα Systems with the Cosmic Origins Spectrograph
DOI: 10.1088/0004-637X/732/1/35 Bibcode: 2011ApJ...732...35M

Sembach, K. R.; Jenkins, E. B.; Prochaska, J. X. +6 more

We report on the first Cosmic Origins Spectrograph observations of damped Lyα systems (DLAs) and sub-damped Lyα systems (sub-DLAs) discovered in a new survey of the gaseous halos of low-redshift galaxies. From observations of 37 sightlines, we have discovered three DLAs and four sub-DLAs. We measure the neutral gas density ΩH I , and re…

2011 The Astrophysical Journal
eHST 77
Possible Charge-exchange X-ray Emission in the Cygnus Loop Detected with Suzaku
DOI: 10.1088/0004-637X/730/1/24 Bibcode: 2011ApJ...730...24K

Katsuda, Satoru; Petre, Robert; Yamaguchi, Hiroya +8 more

X-ray spectroscopic measurements of the Cygnus Loop supernova remnant indicate that metal abundances throughout most of the remnant's rim are depleted to ~0.2 times the solar value. However, recent X-ray studies have revealed in some narrow regions along the outermost rim anomalously "enhanced" abundances (up to ~1 solar). The reason for these ano…

2011 The Astrophysical Journal
Suzaku XMM-Newton 76
Constraints on Coronal Mass Ejection Evolution from in Situ Observations of Ionic Charge States
DOI: 10.1088/0004-637X/730/2/103 Bibcode: 2011ApJ...730..103G

Antiochos, Spiro K.; Zurbuchen, Thomas H.; Gruesbeck, Jacob R. +1 more

We present a novel procedure for deriving the physical properties of coronal mass ejections (CMEs) in the corona. Our methodology uses in situ measurements of ionic charge states of C, O, Si, and Fe in the heliosphere and interprets them in the context of a model for the early evolution of interplanetary CME (ICME) plasma, between 2 and 5 R s…

2011 The Astrophysical Journal
SOHO 76
LYRA Observations of Two Oscillation Modes in a Single Flare
DOI: 10.1088/0004-637X/740/2/90 Bibcode: 2011ApJ...740...90V

Berghmans, D.; Goossens, M.; Zender, J. +2 more

We analyze light curves from the LYRA irradiance experiment on board PROBA2 during the flare of 2010 February 8. We see both long- and short-period oscillations during the flare. The long-period oscillation is interpreted in terms of standing slow sausage modes; the short-period oscillation is thought to be a standing fast sausage mode. The simult…

2011 The Astrophysical Journal
Hinode PROBA-2 75
A Deep Chandra ACIS Study of NGC 4151. III. The Line Emission and Spectral Analysis of the Ionization Cone
DOI: 10.1088/0004-637X/742/1/23 Bibcode: 2011ApJ...742...23W

Elvis, Martin; Zezas, Andreas; Schinnerer, Eva +6 more

This paper is the third in a series in which we present deep Chandra ACIS-S imaging spectroscopy of the Seyfert 1 galaxy NGC 4151, devoted to study its complex circumnuclear X-ray emission. Emission features in the soft X-ray spectrum of the bright extended emission (L 0.3-2 keV ~ 1040 erg s-1) at r > 130 pc (2'…

2011 The Astrophysical Journal
eHST 75
The Variable Quiescent X-Ray Emission of the Transient Neutron Star XTE J1701-462
DOI: 10.1088/0004-637X/736/2/162 Bibcode: 2011ApJ...736..162F

Homan, Jeroen; Cackett, Edward M.; Fridriksson, Joel K. +6 more

We present the results of continued monitoring of the quiescent neutron star low-mass X-ray binary XTE J1701-462 with Chandra and Swift. A new Chandra observation from 2010 October extends our tracking of the neutron star surface temperature from ≃ 800 days to ≃ 1160 days since the end of an exceptionally luminous 19 month outburst. This observati…

2011 The Astrophysical Journal
XMM-Newton 75
Morphological Evolution of Galaxies from Ultra-deep Hubble Space Telescope Wide Field Camera 3 Imaging: The Hubble Sequence at z ~ 2
DOI: 10.1088/2041-8205/735/1/L22 Bibcode: 2011ApJ...735L..22S

van Dokkum, Pieter G.; Franx, Marijn; Illingworth, Garth D. +4 more

We use ultra-deep Hubble Space Telescope Wide Field Camera 3/infrared imaging of the Hubble Ultra Deep Field to investigate the rest-frame optical morphologies of a mass-selected sample of galaxies at z ~ 2. We find a large variety of galaxy morphologies, ranging from large, blue, disk-like galaxies to compact, red, early-type galaxies. We derive …

2011 The Astrophysical Journal
eHST 75
Emission Measure Distribution and Heating of Two Active Region Cores
DOI: 10.1088/0004-637X/740/2/111 Bibcode: 2011ApJ...740..111T

Tripathi, Durgesh; Mason, Helen E.; Klimchuk, James A.

Using data from the Extreme-ultraviolet Imaging Spectrometer aboard Hinode, we have studied the coronal plasma in the core of two active regions. Concentrating on the area between opposite polarity moss, we found emission measure distributions having an approximate power-law form EMvpropT 2.4 from log T = 5.5 up to a peak at log T = 6.5…

2011 The Astrophysical Journal
Hinode SOHO 75
Lyα Emitting Galaxies as Early Stages in Galaxy Formation
DOI: 10.1088/0004-637X/738/2/136 Bibcode: 2011ApJ...738..136C

Cowie, Lennox L.; Barger, Amy J.; Hu, Esther M.

We present optical spectroscopy of two samples of Galaxy Evolution Explorer grism selected Lyα emitters (LAEs): one at z = 0.195-0.44 and the other at z = 0.65-1.25. We have also observed a comparison sample of galaxies in the same redshift intervals with the same UV magnitude distributions but with no detected Lyα. We use the optical spectroscopy…

2011 The Astrophysical Journal
eHST 75