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The Carnegie Hubble Program: The Leavitt Law at 3.6 and 4.5 µm in the Milky Way
DOI: 10.1088/0004-637X/759/2/146 Bibcode: 2012ApJ...759..146M

Madore, Barry F.; Freedman, Wendy L.; Rigby, Jane R. +4 more

The Carnegie Hubble Program (CHP) is designed to calibrate the extragalactic distance scale using data from the post-cryogenic era of the Spitzer Space Telescope. The ultimate goal of the CHP is a systematic improvement in the distance scale leading to a determination of the Hubble constant to within an accuracy of 2%. This paper focuses on the me…

2012 The Astrophysical Journal
eHST 86
The Hubble Wide Field Camera 3 Test of Surfaces in the Outer Solar System: The Compositional Classes of the Kuiper Belt
DOI: 10.1088/0004-637X/749/1/33 Bibcode: 2012ApJ...749...33F

Fraser, Wesley C.; Brown, Michael E.

We present the first results of the Hubble Wide Field Camera 3 Test of Surfaces in the Outer Solar System. The purpose of this survey was to measure the surface properties of a large number of Kuiper Belt objects and attempt to infer compositional and dynamical correlations. We find that the Centaurs and the low-perihelion scattered disk and reson…

2012 The Astrophysical Journal
eHST 85
Numerical Simulations of the Magnetic Rayleigh-Taylor Instability in the Kippenhahn-Schlüter Prominence Model. I. Formation of Upflows
DOI: 10.1088/0004-637X/746/2/120 Bibcode: 2012ApJ...746..120H

Shibata, Kazunari; Isobe, Hiroaki; Hillier, Andrew +1 more

The launch of the Hinode satellite led to the discovery of rising plumes, dark in chromospheric lines, that propagate from large (~10 Mm) bubbles that form at the base of quiescent prominences. The plumes move through a height of approximately 10 Mm while developing highly turbulent profiles. The magnetic Rayleigh-Taylor instability was hypothesiz…

2012 The Astrophysical Journal
Hinode 85
Herschel-SPIRE Imaging Spectroscopy of Molecular Gas in M82
DOI: 10.1088/0004-637X/753/1/70 Bibcode: 2012ApJ...753...70K

Cooray, A.; Isaak, K. G.; Lebouteiller, V. +14 more

We present new Herschel-SPIRE imaging spectroscopy (194-671 µm) of the bright starburst galaxy M82. Covering the CO ladder from J = 4 → 3 to J = 13 → 12, spectra were obtained at multiple positions for a fully sampled ~3 × 3 arcmin map, including a longer exposure at the central position. We present measurements of 12CO, 13

2012 The Astrophysical Journal
Herschel 84
Solar Coronal Loops Resolved by Hinode and the Solar Dynamics Observatory
DOI: 10.1088/2041-8205/755/2/L33 Bibcode: 2012ApJ...755L..33B

Warren, Harry P.; Ugarte-Urra, Ignacio; Brooks, David H.

Despite decades of studying the Sun, the coronal heating problem remains unsolved. One fundamental issue is that we do not know the spatial scale of the coronal heating mechanism. At a spatial resolution of 1000 km or more, it is likely that most observations represent superpositions of multiple unresolved structures. In this Letter, we use a comb…

2012 The Astrophysical Journal
Hinode 83
The SL2S Galaxy-scale Gravitational Lens Sample. I. The Alignment of Mass and Light in Massive Early-type Galaxies at z = 0.2-0.9
DOI: 10.1088/0004-637X/761/2/170 Bibcode: 2012ApJ...761..170G

Treu, Tommaso; Gavazzi, Raphaël; Marshall, Philip J. +2 more

We study the relative alignment of mass and light in a sample of 16 massive early-type galaxies at z = 0.2-0.9 that act as strong gravitational lenses. The sample was identified from deep multi-band images obtained as part of the Canada-France-Hawaii Telescope Legacy Survey and as part of the Strong Lensing Legacy Survey (SL2S). Higher resolution …

2012 The Astrophysical Journal
eHST 83
The Relation between Cool Cluster Cores and Herschel-detected Star Formation in Brightest Cluster Galaxies
DOI: 10.1088/0004-637X/747/1/29 Bibcode: 2012ApJ...747...29R

Smith, G. P.; Altieri, B.; Valtchanov, I. +12 more

We present far-infrared (FIR) analysis of 68 brightest cluster galaxies (BCGs) at 0.08 < z < 1.0. Deriving total infrared luminosities directly from Spitzer and Herschel photometry spanning the peak of the dust component (24-500 µm), we calculate the obscured star formation rate (SFR). 22+6.2 -5.3% of the BCGs are…

2012 The Astrophysical Journal
Herschel eHST 83
Supergranules as Probes of the Sun's Meridional Circulation
DOI: 10.1088/0004-637X/760/1/84 Bibcode: 2012ApJ...760...84H

Hathaway, David H.

Recent analysis revealed that supergranules (convection cells seen at the Sun's surface) are advected by the zonal flows at depths equal to the widths of the cells themselves. Here we probe the structure of the meridional circulation by cross-correlating maps of the Doppler velocity signal using a series of successively longer time lags between ma…

2012 The Astrophysical Journal
SOHO 83
On the Nature of the Solar Wind from Coronal Pseudostreamers
DOI: 10.1088/0004-637X/749/2/182 Bibcode: 2012ApJ...749..182W

Sheeley, N. R., Jr.; Wang, Y. -M.; Robbrecht, E. +1 more

Coronal pseudostreamers, which separate like-polarity coronal holes, do not have current sheet extensions, unlike the familiar helmet streamers that separate opposite-polarity holes. Both types of streamers taper into narrow plasma sheets that are maintained by continual interchange reconnection with the adjacent open magnetic field lines. White-l…

2012 The Astrophysical Journal
SOHO 83
Submillimeter Line Spectrum of the Seyfert Galaxy NGC 1068 from the Herschel-SPIRE Fourier Transform Spectrometer
DOI: 10.1088/0004-637X/758/2/108 Bibcode: 2012ApJ...758..108S

Wilson, Christine D.; Bendo, George J.; Madden, Suzanne C. +13 more

The first complete submillimeter spectrum (190-670 µm) of the Seyfert 2 galaxy NGC 1068 has been observed with the SPIRE Fourier transform spectrometer on board the Herschel Space Observatory. The sequence of CO lines (J up = 4-13), lines from H2O, the fundamental rotational transition of hydrogen fluoride, two o-H

2012 The Astrophysical Journal
Herschel 83