Search Publications

Automated Detection of Galaxy-Scale Gravitational Lenses in High-Resolution Imaging Data
DOI: 10.1088/0004-637X/694/2/924 Bibcode: 2009ApJ...694..924M

Bradač, Maruša; Hogg, David W.; Marshall, Philip J. +4 more

We expect direct lens modeling to be the key to successful and meaningful automated strong galaxy-scale gravitational lens detection. We have implemented a lens-modeling "robot" that treats every bright red galaxy (BRG) in a large imaging survey as a potential gravitational lens system. Having optimized a simple model for "typical" galaxy-scale gr…

2009 The Astrophysical Journal
eHST 74
The Expanding Nebular Remnant of the Recurrent Nova RS Ophiuchi (2006). II. Modeling of Combined Hubble Space Telescope Imaging and Ground-based Spectroscopy
DOI: 10.1088/0004-637X/703/2/1955 Bibcode: 2009ApJ...703.1955R

Chavushyan, V. H.; Zharikov, S. V.; Eyres, S. P. S. +16 more

We report Hubble Space Telescope (HST) imaging, obtained 155 and 449 days after the 2006 outburst of the recurrent nova RS Ophiuchi, together with ground-based spectroscopic observations, obtained from the Observatorio Astronómico Nacional en San Pedro Mártir, Baja California, México and at the Observatorio Astrofísico Guillermo Haro, at Cananea, …

2009 The Astrophysical Journal
eHST 74
A "Firework" of H2 Knots in the Planetary Nebula NGC 7293 (The Helix Nebula)
DOI: 10.1088/0004-637X/700/2/1067 Bibcode: 2009ApJ...700.1067M

Smith, M. D.; Tanaka, I.; Zijlstra, A. A. +6 more

We present a deep and wide field-of-view (4' × 7') image of the planetary nebula (PN) NGC 7293 (the Helix Nebula) in the 2.12 µm H2 v = 1 → 0 S(1) line. The excellent seeing (0farcs4) at the Subaru Telescope, allows the details of cometary knots to be examined. The knots are found at distances of 2farcm2-6farcm4 from the central s…

2009 The Astrophysical Journal
eHST 73
Detection of Water Ice Grains on the Surface of the Circumstellar Disk Around HD 142527
DOI: 10.1088/0004-637X/690/2/L110 Bibcode: 2009ApJ...690L.110H

Tamura, M.; Ishii, M.; Kudo, T. +11 more

Coronagraphic imaging for the Herbig Ae star, HD 142527, was performed using the Coronagraphic Imager with Adaptive Optics (CIAO) on the 8.2 m Subaru Telescope. The images were obtained in the H2O ice filter (λ = 3.08 µm) using adaptive optics (AO), and in the L' band without AO. Combining these data with previous observational re…

2009 The Astrophysical Journal
ISO 73
NTT, Spitzer, and Chandra Spectroscopy of SDSSJ095209.56+214313.3: The Most Luminous Coronal-line Supernova Ever Observed, or a Stellar Tidal Disruption Event?
DOI: 10.1088/0004-637X/701/1/105 Bibcode: 2009ApJ...701..105K

Greiner, J.; Gal-Yam, A.; Salvato, M. +9 more

The galaxy SDSSJ095209.56+214313.3 (SDSSJ0952+2143 hereafter) showed remarkable emission-line and continuum properties and strong emission-line variability first reported in 2008 (Paper I). The spectral properties and low-energy variability are the consequence of a powerful high-energy flare which was itself not observed directly. Here we report f…

2009 The Astrophysical Journal
XMM-Newton 73
Modulation of Galactic Cosmic Ray Protons and Electrons During an Unusual Solar Minimum
DOI: 10.1088/0004-637X/699/2/1956 Bibcode: 2009ApJ...699.1956H

Fichtner, H.; Scherer, K.; Ferreira, S. E. S. +5 more

During the latest Ulysses out-of-ecliptic orbit the solar wind density, pressure, and magnetic field strength have been the lowest ever observed in the history of space exploration. Since cosmic ray particles respond to the heliospheric magnetic field in the expanding solar wind and its turbulence, the weak heliospheric magnetic field as well as t…

2009 The Astrophysical Journal
Ulysses 73
The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. III. More Results From the Magellanic Clouds
DOI: 10.1088/0004-637X/692/1/618 Bibcode: 2009ApJ...692..618M

Massey, Philip; Bresolin, Fabio; Kudritzki, Rolf-Peter +4 more

In order to better determine the physical properties of hot, massive stars as a function of metallicity, we obtained very high signal-to-noise ratio optical spectra of 26 O and early B stars in the Magellanic Clouds. These allow accurate modeling even in cases where the He I λ4471 line has an equivalent width of only a few tens of m Å. The spectra…

2009 The Astrophysical Journal
eHST 73
Spatially Resolved Spectroscopy of Sub-AU-Sized Regions of T Tauri and Herbig Ae/Be Disks
DOI: 10.1088/0004-637X/692/1/309 Bibcode: 2009ApJ...692..309E

Najita, J.; Eisner, J. A.; Graham, J. R. +1 more

We present spatially resolved near-IR spectroscopic observations of 15 young stars. Using a grism spectrometer behind the Keck interferometer, we obtained an angular resolution of a few milliarcseconds and a spectral resolution of 230, enabling probes of both gas and dust in the inner disks surrounding the target stars. We find that the angular si…

2009 The Astrophysical Journal
ISO 72
The True Durations of Starbursts: Hubble Space Telescope Observations of Three Nearby Dwarf Starburst Galaxies
DOI: 10.1088/0004-637X/695/1/561 Bibcode: 2009ApJ...695..561M

McQuinn, Kristen B. W.; Cannon, John M.; Skillman, Evan D. +4 more

The duration of a starburst is a fundamental parameter affecting the evolution of galaxies yet, to date, observational constraints on the durations of starbursts are not well established. Here we study the recent star formation histories of three nearby dwarf galaxies to rigorously quantify the duration of their starburst events using a uniform an…

2009 The Astrophysical Journal
eHST 72
Keck Laser Guide Star Adaptive Optics Monitoring of the M8+L7 Binary LHS 2397aAB: First Dynamical Mass Benchmark at the L/T Transition
DOI: 10.1088/0004-637X/699/1/168 Bibcode: 2009ApJ...699..168D

Dupuy, Trent J.; Ireland, Michael J.; Liu, Michael C.

We present Keck laser guide star adaptive optics imaging and aperture masking observations of the M8+L7 binary LHS 2397aAB. Together with archival Hubble Space Telescope, Gemini-North, and Very Large Telescope data, our observations span 11.8 years of the binary's 14.2 year orbital period. We determine a total dynamical mass of 0.146+0.015

2009 The Astrophysical Journal
eHST 72