Search Publications

The Anatomy of Star Formation in NGC 300
DOI: 10.1086/422640 Bibcode: 2004ApJS..154..253H

Helou, G.; Roussel, H.; Fazio, G. G. +19 more

The Spitzer Space Telescope was used to study the mid- to far-infrared properties of NGC 300 and to compare dust emission to Hα to elucidate the heating of the interstellar medium (ISM) and the star formation cycle at scales smaller than 100 pc. The new data allow us to discern clear differences in the spatial distribution of 8 µm dust emiss…

2004 The Astrophysical Journal Supplement Series
ISO 259
An Extended Scheme for Fitting X-Ray Data with Accretion Disk Spectra in the Strong Gravity Regime
DOI: 10.1086/421115 Bibcode: 2004ApJS..153..205D

Yaqoob, T.; Dovčiak, M.; Karas, V.

Accreting black holes are believed to emit X-rays, which then mediate information about strong gravity in the vicinity of the emission region. We report on a set of new routines for the XSPEC package for analyzing X-ray spectra of black-hole accretion disks. The new computational tool significantly extends the capabilities of the currently availab…

2004 The Astrophysical Journal Supplement Series
XMM-Newton 253
The Rest-Frame Optical Spectra of SCUBA Galaxies
DOI: 10.1086/425171 Bibcode: 2004ApJ...617...64S

Ivison, R. J.; Smail, Ian; Swinbank, A. M. +3 more

We present near-infrared spectroscopy and narrowband imaging at the wavelength of redshifted Hα for a sample of 30 high-redshift, far-infrared luminous galaxies. This sample is selected from surveys in the submillimeter, millimeter, and radio wave bands and has complete redshift coverage with a median redshift of z~2.4. We use our data to measure …

2004 The Astrophysical Journal
eHST 251
A Study of the Kinematic Evolution of Coronal Mass Ejections
DOI: 10.1086/381725 Bibcode: 2004ApJ...604..420Z

Zhang, J.; Howard, R. A.; Dere, K. P. +1 more

We report the kinematic properties of a set of three coronal mass ejections (CMEs) observed with the LASCO (Large Angle and Spectrometric Coronagraph) on the Solar and Heliospheric Observatory (SOHO) spacecraft, which showed characteristics of impulsive, intermediate, and gradual acceleration, respectively. The first CME had a 30 minute long fast …

2004 The Astrophysical Journal
SOHO 250
Constraining the population of cosmic ray protons in cooling flow clusters with γ-ray and radio observations: Are radio mini-halos of hadronic origin?
DOI: 10.1051/0004-6361:20031464 Bibcode: 2004A&A...413...17P

Enßlin, T. A.; Pfrommer, C.

We wish to constrain the cosmic-ray proton (CRp) population in galaxy clusters. By hadronic interactions with the thermal gas of the intra-cluster medium (ICM), the CRp produce γ-rays for which we develop an analytic formalism to deduce their spectral distribution. Assuming the CRp-to-thermal energy density ratio XCRp and the CRp spectr…

2004 Astronomy and Astrophysics
INTEGRAL 249
Galaxy Size Evolution at High Redshift and Surface Brightness Selection Effects: Constraints from the Hubble Ultra Deep Field
DOI: 10.1086/423786 Bibcode: 2004ApJ...611L...1B

Bouwens, R. J.; Illingworth, G. D.; Blakeslee, J. P. +2 more

We use the exceptional depth of the Ultra Deep Field (UDF) and UDF-parallel Advanced Camera for Surveys fields to study the sizes of high-redshift (z~2-6) galaxies and address long-standing questions about possible biases in the cosmic star formation rate due to surface brightness dimming. Contrasting B-, V-, and i-dropout samples culled from the …

2004 The Astrophysical Journal
eHST 247
Cone model for halo CMEs: Application to space weather forecasting
DOI: 10.1029/2003JA010226 Bibcode: 2004JGRA..109.3109X

Xie, Hong; Ofman, Leon; Lawrence, Gareth

In this study, we present an innovative analytical method to determine the angular width and propagation orientation of halo Coronal Mass Ejections (CMEs). The relation of CME actual speed with apparent speed and its components measured at different position angle has been investigated. The present work is based on the cone model proposed by [2002…

2004 Journal of Geophysical Research (Space Physics)
SOHO 247
Constraining Solar Abundances Using Helioseismology
DOI: 10.1086/421110 Bibcode: 2004ApJ...606L..85B

Basu, Sarbani; Antia, H. M.

Recent analyses of solar photospheric abundances suggest that the oxygen abundance in the solar atmosphere needs to be revised downward. In this study, we investigate the consequence of this revision on helioseismic analyses of the depth of the solar convection zone and the helium abundance in the solar envelope and find no significant effect. We …

2004 The Astrophysical Journal
SOHO 245
Star formation history and dust content of galaxies drawn from ultraviolet surveys
DOI: 10.1111/j.1365-2966.2004.07556.x Bibcode: 2004MNRAS.349..769K

Kong, X.; Brinchmann, J.; Charlot, S. +1 more

We compile a new sample of 115 nearby, non-Seyfert galaxies spanning a wide range of star formation activities, from starburst to nearly dormant, based on ultraviolet observations with various satellites. We combine these observations with infrared observations to study the relation between ratio of total far-infrared to ultraviolet luminosity and…

2004 Monthly Notices of the Royal Astronomical Society
IUE 245
High-Redshift Supernova Rates
DOI: 10.1086/422899 Bibcode: 2004ApJ...613..189D

Ferguson, Henry C.; Giavalisco, Mauro; Fruchter, Andrew S. +10 more

We use a sample of 42 supernovae detected with the Advanced Camera for Surveys on board the Hubble Space Telescope as part of the Great Observatories Origins Deep Survey to measure the rate of core-collapse supernovae to z~0.7 and Type Ia supernovae to z~1.6. This significantly increases the redshift range at which supernova rates have been estima…

2004 The Astrophysical Journal
eHST 244