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Globular Cluster Systems in Brightest Cluster Galaxies: Bimodal Metallicity Distributions and the Nature of the High-Luminosity Clusters
DOI: 10.1086/498058 Bibcode: 2006ApJ...636...90H

Whitmore, Bradley C.; Kavelaars, J. J.; Baum, William A. +4 more

We present new (B, I) photometry for the globular cluster systems in eight brightest cluster galaxies (BCGs), obtained with the ACS/WFC camera on the Hubble Space Telescope. In the very rich cluster systems that reside within these giant galaxies, we find that all have strongly bimodal color distributions that are clearly resolved by the metallici…

2006 The Astrophysical Journal
eHST 195
Near-Infrared and Star-forming Properties of Local Luminous Infrared Galaxies
DOI: 10.1086/506958 Bibcode: 2006ApJ...650..835A

Pérez-González, Pablo G.; Ryder, Stuart D.; Colina, Luis +3 more

We use Hubble Space Telescope (HST) NICMOS continuum and Paα observations to study the near-infrared and star formation properties of a representative sample of 30 local (d~35-75 Mpc) luminous infrared galaxies (LIRGs, infrared [8-1000 µm] luminosities of logLIR=11-11.9 Lsolar). The data provide spatial resolutions of 2…

2006 The Astrophysical Journal
eHST 195
Light neutralino dark matter in the next-to-minimal supersymmetric standard model
DOI: 10.1103/PhysRevD.73.015011 Bibcode: 2006PhRvD..73a5011G

Hooper, Dan; Gunion, John F.; McElrath, Bob

Neutralino dark matter is generally assumed to be relatively heavy, with a mass near the electroweak scale. This does not necessarily need to be the case, however. In the next-to-minimal supersymmetric standard model (NMSSM) and other supersymmetric models with an extended Higgs sector, a very light CP-odd Higgs boson can naturally arise making it…

2006 Physical Review D
INTEGRAL 195
The great observatories origins deep survey. VLT/FORS2 spectroscopy in the GOODS-South Field: Part II
DOI: 10.1051/0004-6361:20054796 Bibcode: 2006A&A...454..423V

Popesso, P.; Cesarsky, C.; Stern, D. +16 more

Aims.We present the second campaign of the ESO/GOODS program of spectroscopy of faint galaxies in the GOODS-South field.
Methods: .Objects were selected as candidates for VLT/FORS2 observations primarily based on the expectation that the detection and measurement of their spectral features would benefit from the high throughput and spectral re…

2006 Astronomy and Astrophysics
eHST 195
Magnetoacoustic Portals and the Basal Heating of the Solar Chromosphere
DOI: 10.1086/508165 Bibcode: 2006ApJ...648L.151J

McIntosh, Scott W.; Cacciani, Alessandro; Armstrong, James D. +3 more

We show that inclined magnetic field lines at the boundaries of large-scale convective cells (supergranules) provide ``portals'' through which low-frequency (<5 mHz) magnetoacoustic waves can propagate into the solar chromosphere. The energy flux carried by these waves at a height of 400 km above the solar surface is found to be a factor of 4 g…

2006 The Astrophysical Journal
SOHO 194
The N2K Consortium. IV. New Temperatures and Metallicities for More than 100,000 FGK Dwarfs
DOI: 10.1086/498490 Bibcode: 2006ApJ...638.1004A

Strader, Jay; Laughlin, Gregory; Ammons, S. Mark +3 more

We have created specialized target lists for radial velocity surveys that are biased toward stars that (1) possess planets and (2) are easiest to observe with current detection techniques. We use a procedure that uniformly estimates fundamental stellar properties of Tycho 2 stars, with errors, using spline functions of broadband photometry and pro…

2006 The Astrophysical Journal
Hipparcos 194
The link between submillimetre galaxies and luminous ellipticals: near-infrared IFU spectroscopy of submillimetre galaxies
DOI: 10.1111/j.1365-2966.2006.10673.x Bibcode: 2006MNRAS.371..465S

Ivison, R. J.; Smail, Ian; Swinbank, A. M. +5 more

We present two-dimensional spectroscopy covering the rest-frame wavelengths of strong optical emission lines in six luminous submillimetre galaxies (SMGs) at z = 1.3-2.5. Using this near-infrared integral field spectroscopy together with Hubble Space Telescope ACS and NICMOS imaging, we map the dynamics and morphologies of these systems on scales …

2006 Monthly Notices of the Royal Astronomical Society
eHST 194
The Hard X-Ray Spectral Slope as an Accretion Rate Indicator in Radio-quiet Active Galactic Nuclei
DOI: 10.1086/506911 Bibcode: 2006ApJ...646L..29S

Maiolino, Roberto; Brandt, W. N.; Kaspi, Shai +2 more

We present new XMM-Newton observations of two luminous and high accretion rate radio-quiet active galactic nuclei (AGNs) at z~2. Together with archival X-ray and rest-frame optical spectra of three sources with similar properties, as well as 25 moderate-luminosity radio-quiet AGNs at z<0.5, we investigate, for the first time, the dependence of …

2006 The Astrophysical Journal
XMM-Newton 194
Hubble Space Telescope STIS Spectra of Nuclear Star Clusters in Spiral Galaxies: Dependence of Age and Mass on Hubble Type
DOI: 10.1086/505968 Bibcode: 2006AJ....132.1074R

Böker, Torsten; Ho, Luis C.; Shields, Joseph C. +5 more

We study the nuclear star clusters (NCs) in spiral galaxies of various Hubble types using spectra obtained with the STIS on board the Hubble Space Telescope (HST). We observed the nuclear clusters in 40 galaxies, selected from two previous HST WFPC2 imaging surveys. At a spatial resolution of ~0.2" the spectra provide a better separation of cluste…

2006 The Astronomical Journal
eHST 194
The Proper Treatment of Coronal Mass Ejection Brightness: A New Methodology and Implications for Observations
DOI: 10.1086/501122 Bibcode: 2006ApJ...642.1216V

Vourlidas, Angelos; Howard, Russell A.

With the complement of coronagraphs and imagers in the SECCHI suite, we will follow a coronal mass ejection (CME) continuously from the Sun to Earth for the first time. The comparison, however, of the CME emission among the various instruments is not as easy as one might think. This is because the telescopes record the Thomson-scattered emission f…

2006 The Astrophysical Journal
SOHO 194