Search Publications

On the Cluster Physics of Sunyaev-Zel'dovich and X-Ray Surveys. I. The Influence of Feedback, Non-thermal Pressure, and Cluster Shapes on Y-M Scaling Relations
DOI: 10.1088/0004-637X/758/2/74 Bibcode: 2012ApJ...758...74B

Bond, J. R.; Battaglia, N.; Sievers, J. L. +1 more

The utility of large Sunyaev-Zel'dovich (SZ) surveys for determining cosmological parameters from cluster abundances is limited by the theoretical uncertainties in the integrated SZ-flux-to-mass relation, Y-M. We explore how non-thermal pressure and the anisotropic shape of the gas distribution of the intracluster medium (ICM) impacts Y-M scaling …

2012 The Astrophysical Journal
Planck 231
A Cool Dust Factory in the Crab Nebula: A Herschel Study of the Filaments
DOI: 10.1088/0004-637X/760/1/96 Bibcode: 2012ApJ...760...96G

Ivison, R. J.; Henning, Th.; Krause, O. +13 more

Whether supernovae are major sources of dust in galaxies is a long-standing debate. We present infrared and submillimeter photometry and spectroscopy from the Herschel Space Observatory of the Crab Nebula between 51 and 670 µm as part of the Mass Loss from Evolved StarS program. We compare the emission detected with Herschel with multiwavele…

2012 The Astrophysical Journal
Herschel ISO Planck 177
Cosmic Microwave Background Constraints on the Duration and Timing of Reionization from the South Pole Telescope
DOI: 10.1088/0004-637X/756/1/65 Bibcode: 2012ApJ...756...65Z

Doré, O.; Bleem, L. E.; Stark, A. A. +48 more

The epoch of reionization is a milestone of cosmological structure formation, marking the birth of the first objects massive enough to yield large numbers of ionizing photons. However, the mechanism and timescale of reionization remain largely unknown. Measurements of the cosmic microwave background (CMB) Doppler effect from ionizing bubbles embed…

2012 The Astrophysical Journal
Planck 148
Can Dust Emission be Used to Estimate the Mass of the Interstellar Medium in Galaxies—A Pilot Project with the Herschel Reference Survey
DOI: 10.1088/0004-637X/761/2/168 Bibcode: 2012ApJ...761..168E

Gear, Walter; Wilson, Christine D.; De Looze, Ilse +23 more

The standard method for estimating the mass of the interstellar medium (ISM) in a galaxy is to use the 21 cm line to trace the atomic gas and the CO 1-0 line to trace the molecular gas. In this paper, we investigate the alternative technique of using the continuum dust emission to estimate the mass of gas in all phases of the ISM. Using Herschel o…

2012 The Astrophysical Journal
Herschel Planck 106
A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy
DOI: 10.1088/0004-637X/753/2/134 Bibcode: 2012ApJ...753..134F

Smail, I.; Pérez-Fournon, I.; Ivison, R. J. +48 more

We present high-resolution maps of stars, dust, and molecular gas in a strongly lensed submillimeter galaxy (SMG) at z = 3.259. HATLAS J114637.9-001132 is selected from the Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) as a strong lens candidate mainly based on its unusually high 500 µm flux density (~300 mJy). It is the only …

2012 The Astrophysical Journal
Herschel Planck 101
Evidence for Environmental Changes in the Submillimeter Dust Opacity
DOI: 10.1088/0004-637X/751/1/28 Bibcode: 2012ApJ...751...28M

Devlin, Mark J.; Halpern, Mark; Miville-Deschênes, Marc-Antoine +25 more

The submillimeter opacity of dust in the diffuse interstellar medium (ISM) in the Galactic plane has been quantified using a pixel-by-pixel correlation of images of continuum emission with a proxy for column density. We used multi-wavelength continuum data: three Balloon-borne Large Aperture Submillimeter Telescope bands at 250, 350, and 500 &micr…

2012 The Astrophysical Journal
Planck 87
The Submillimeter and Millimeter Excess of the Small Magellanic Cloud: Magnetic Dipole Emission from Magnetic Nanoparticles?
DOI: 10.1088/0004-637X/757/1/103 Bibcode: 2012ApJ...757..103D

Hensley, Brandon; Draine, B. T.

The Small Magellanic Cloud (SMC) has surprisingly strong submillimeter- and millimeter-wavelength emission that is inconsistent with standard dust models, including those with emission from spinning dust. Here, we show that the emission from the SMC may be understood if the interstellar dust mixture includes magnetic nanoparticles, emitting magnet…

2012 The Astrophysical Journal
Planck 79
Gas Emissions in Planck Cold Dust Clumps—A Survey of the J = 1-0 Transitions of 12CO, 13CO, and C18O
DOI: 10.1088/0004-637X/756/1/76 Bibcode: 2012ApJ...756...76W

Li, Di; Liu, Tie; Qin, Sheng-Li +3 more

A survey toward 674 Planck cold clumps of the Early Cold Core Catalogue (ECC) in the J = 1-0 transitions of 12CO, 13CO, and C18O has been carried out using the Purple Mountain Observatory 13.7 m telescope. Six hundred seventy-three clumps were detected with 12CO and 13CO emission, and 68% of t…

2012 The Astrophysical Journal
Planck 73
Herschel PACS and SPIRE Observations of Blazar PKS 1510-089: A Case for Two Blazar Zones
DOI: 10.1088/0004-637X/760/1/69 Bibcode: 2012ApJ...760...69N

Szczerba, Ryszard; Nalewajko, Krzysztof; Madejski, Greg M. +5 more

We present the results of observations of blazar PKS 1510-089 with the Herschel Space Observatory PACS and SPIRE instruments, together with multiwavelength data from Fermi/LAT, Swift, SMARTS, and Submillimeter Array. The source was found in a quiet state, and its far-infrared spectrum is consistent with a power law with a spectral index of α ~= 0.…

2012 The Astrophysical Journal
Herschel Planck 54
The Y SZ-YX Scaling Relation as Determined from Planck and Chandra
DOI: 10.1088/0004-637X/760/1/67 Bibcode: 2012ApJ...760...67R

Vikhlinin, Alexey; More, Surhud; Rozo, Eduardo

Sunyaev-Zeldovich (SZ) clusters surveys, such as Planck, the South Pole Telescope, and the Atacama Cosmology Telescope, will soon be publishing several hundred SZ-selected systems. The key ingredient required to transport the mass calibration from current X-ray-selected cluster samples to these SZ systems is the Y SZ-YX scali…

2012 The Astrophysical Journal
Planck 31