Search Publications

Submillimeter Array Imaging of the CO(3-2) Line and 860 µm Continuum of Arp 220: Tracing the Spatial Distribution of Luminosity
DOI: 10.1086/590484 Bibcode: 2008ApJ...684..957S

Wilner, David J.; Zhang, Qizhou; Wang, Junzhi +6 more

We used the Submillimeter Array (SMA) to image 860 µm continuum and CO(3-2) line emission in the ultraluminous merging galaxy Arp 220, achieving a resolution of 0.23'' (80 pc) for the continuum and 0.33'' (120 pc) for the line. The CO emission peaks around the two merger nuclei with a velocity signature of gas rotation …

2008 The Astrophysical Journal
eHST 126
Separating Baryons and Dark Matter in Cluster Cores: A Full Two-dimensional Lensing and Dynamic Analysis of Abell 383 and MS 2137-23
DOI: 10.1086/524652 Bibcode: 2008ApJ...674..711S

Smith, Graham P.; Treu, Tommaso; Ellis, Richard S. +2 more

We utilize existing data for the galaxy clusters MS 2137-23 and Abell 383 to present improved measures of the distribution of dark and baryonic material in the clusters' central regions. Our method, based on the combination of gravitational lensing and dynamical data, is uniquely capable of separating the distribution of dark and baryonic componen…

2008 The Astrophysical Journal
eHST 124
Spatially Resolved Properties of the GRB 060505 Host: Implications for the Nature of the Progenitor
DOI: 10.1086/528943 Bibcode: 2008ApJ...676.1151T

Fruchter, Andrew S.; Östlin, Göran; Hjorth, Jens +12 more

GRB 060505 was the first well-observed nearby possible long-duration gamma-ray burst (GRB) that had no associated supernova. Here we present spatially resolved spectra of the host galaxy of GRB 060505, an Sbc spiral, at redshift z = 0.0889. The GRB occurred inside a star-forming region in the northern spiral arm at 6.5 kpc from the center. From th…

2008 The Astrophysical Journal
eHST 123
Resonant Cyclotron Scattering in Magnetars' Emission
DOI: 10.1086/591264 Bibcode: 2008ApJ...686.1245R

Götz, D.; Rea, N.; Lyutikov, M. +2 more

We present a systematic fit of a model of resonant cyclotron scattering (RCS) to the X-ray data of 10 magnetars, including canonical and transient anomalous X-ray pulsars (AXPs) and soft gamma repeaters (SGRs). In this scenario, nonthermal magnetar spectra in the soft X-rays (i.e., below ~10 keV) result from resonant cyclotron scattering of the th…

2008 The Astrophysical Journal
INTEGRAL XMM-Newton 123
Modeling Fe II Emission and Revised Fe II (UV) Empirical Templates for the Seyfert 1 Galaxy I Zw 1
DOI: 10.1086/525557 Bibcode: 2008ApJ...675...83B

Bruhweiler, F.; Verner, E.

We use the narrow-lined broad-line region (BLR) of the Seyfert 1 galaxy, I Zw 1, as a laboratory for modeling the ultraviolet (UV) Fe II 2100-3050 Å emission complex. We calculate a grid of Fe II emission spectra representative of BLR clouds and compare them with the observed I Zw 1 spectrum. Our predicted spectrum for log [nH/(cm

2008 The Astrophysical Journal
eHST 122
The Detailed Evolution of E+A Galaxies into Early Types
DOI: 10.1086/591656 Bibcode: 2008ApJ...688..945Y

Zabludoff, Ann I.; Zaritsky, Dennis; Yang, Yujin +1 more

Poststarburst, or E+A, galaxies are the best candidates for galaxies in transition from being gas-rich and star-forming to gas-poor and passively evolving as a result of galaxy-galaxy interactions. To focus on what E+A galaxies become after their young stellar populations fade away, we present the detailed morphologies of 21 E+A galaxies using hig…

2008 The Astrophysical Journal
eHST 121
Spectroscopic Confirmation of an Extreme Starburst at Redshift 4.547
DOI: 10.1086/590555 Bibcode: 2008ApJ...681L..53C

Aussel, H.; Sanders, D. B.; Ilbert, O. +22 more

We report the spectroscopic confirmation of a submillimeter galaxy (SMG) at z = 4.547 with an estimated LIR = (0.5-2.0) × 1013 L. The spectra, mid-IR, and X-ray properties indicate the bolometric luminosity is dominated by star formation at a rate of >1000 M yr-1. Multiple, spatially sepa…

2008 The Astrophysical Journal
eHST 121
Lyman Break Galaxies, Lyα Emitters, and a Radio Galaxy in a Protocluster at z = 4.1
DOI: 10.1086/524342 Bibcode: 2008ApJ...673..143O

Ford, H. C.; Demarco, R.; Zheng, W. +17 more

We present deep HST ACS observations in g475r625i775z850 toward the z = 4.1 radio galaxy TN J1338-1942 and its overdensity of >30 spectroscopically confirmed Lyα emitters (LAEs). We select 66 g475 band dropouts to z850,5 σ = 27, 6 of which are also LAEs. Although our color-color …

2008 The Astrophysical Journal
eHST 120
Exoplanet HD 209458b (Osiris): Evaporation Strengthened
DOI: 10.1086/587036 Bibcode: 2008ApJ...676L..57V

Lecavelier des Etangs, A.; Ferlet, R.; Vidal-Madjar, A. +4 more

Following reanalysis of Hubble Space Telescope observations of primary transits of the extrasolar planet HD 209458b at Lyα, Ben-Jaffel claims that no sign of evaporation is observed. Here we show that, in fact, this new analysis is consistent with the one of Vidal-Madjar and coworkers, and supports the detection of evaporation. The apparent disagr…

2008 The Astrophysical Journal
eHST 120
A Global Kinetic Model for Cometary Comae: The Evolution of the Coma of the Rosetta Target Comet Churyumov-Gerasimenko throughout the Mission
DOI: 10.1086/590376 Bibcode: 2008ApJ...685..659T

Tenishev, Valeriy; Combi, Michael; Davidsson, Björn

The Rosetta spacecraft is en route to comet 67P/Churyumov-Gerasimenko for a rendezvous, landing, and extensive orbital phase beginning in 2014. Model studies of the coma will be required not only for planning of the mission and interpretation of spacecraft data, but also for an expectedly large amount of complementary remote observational data tha…

2008 The Astrophysical Journal
Rosetta 119