Search Publications

Evidence of a Significant Intermediate-Age Population in the M31 Halo from Main-Sequence Photometry
DOI: 10.1086/376935 Bibcode: 2003ApJ...592L..17B

Ferguson, Henry C.; Brown, Thomas M.; Rich, R. Michael +5 more

We present a color-magnitude diagram (CMD) for a minor-axis field in the halo of the Andromeda galaxy (M31), 51' (11 kpc) from the nucleus. These observations, taken with the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope, are the deepest optical images yet obtained, attaining 50% completeness at mV=30.7 mag. The CMD, c…

2003 The Astrophysical Journal
eHST 142
Discovery of Interacting Molecular Gas toward the TeV Gamma-Ray Peak of the SNR G 347.3--0.5
DOI: 10.1093/pasj/55.5.L61 Bibcode: 2003PASJ...55L..61F

Takahashi, Tadayuki; Uchiyama, Yasunobu; Fukui, Yasuo +10 more

Supernova remnants ( = SNR) are suggested to be sites of cosmic-ray acceleration. In particular, it has been an issue of keen interest whether cosmic ray protons are being accelerated in a SNR which emits TeV γ-rays. A crucial observational test for this is to find dense molecular gas towards the SNR, because such molecular gas can best verify the…

2003 Publications of the Astronomical Society of Japan
XMM-Newton 141
The Initial Helium Content of Galactic Globular Cluster Stars from the R-Parameter: Comparison with the Cosmic Microwave Background Constraint
DOI: 10.1086/374218 Bibcode: 2003ApJ...588..862C

Salaris, Maurizio; Cassisi, Santi; Irwin, Alan W.

Recent precise determinations of the primordial He abundance (Yp) from cosmic microwave background (CMB) analyses and cosmological nucleosynthesis computations provide Yp=0.248+/-0.001. On the other hand, recent works on the initial He abundance of Galactic globular cluster (GGC) stars, making use of the R-parameter as an He …

2003 The Astrophysical Journal
eHST 141
The Hubble Constant from the Gravitational Lens B1608+656
DOI: 10.1086/379226 Bibcode: 2003ApJ...599...70K

Treu, T.; Blandford, R. D.; Koopmans, L. V. E. +2 more

We present a refined gravitational lens model of the four-image lens system B1608+656 based on new and improved observational constraints: (1) the three independent time delays and flux ratios from Very Large Array observations, (2) the radio-image positions from Very Large Baseline Array observations, (3) the shape of the deconvolved Einstein rin…

2003 The Astrophysical Journal
eHST 141
Multiple magnetic clouds: Several examples during March-April 2001
DOI: 10.1029/2003JA009850 Bibcode: 2003JGRA..108.1370W

Wang, S.; Wang, Y. M.; Ye, P. Z.

Multiple magnetic cloud (Multi-MC), which is formed by the overtaking of successive coronal mass ejections (CMEs), is a kind of complex structure in interplanetary space. Multi-MC is worthy of notice due to its special properties and potential geoeffectiveness. Using the data from the ACE spacecraft, we identify the three cases of Multi-MC in the …

2003 Journal of Geophysical Research (Space Physics)
SOHO 141
Hubble Space Telescope Imaging of Brightest Cluster Galaxies
DOI: 10.1086/345823 Bibcode: 2003AJ....125..478L

O'Dea, Christopher P.; van der Marel, Roeland P.; Lauer, Tod R. +3 more

We used the Hubble Space Telescope Wide Field Planetary Camera 2 to obtain I-band images of the centers of 81 brightest cluster galaxies (BCGs), drawn from a volume-limited sample of nearby BCGs. The images show a rich variety of morphological features, including multiple or double nuclei, dust, stellar disks, point-source nuclei, and central surf…

2003 The Astronomical Journal
eHST 139
Giant Lyα Nebulae Associated with High-Redshift Radio Galaxies
DOI: 10.1086/375619 Bibcode: 2003ApJ...592..755R

Dey, Arjun; Bland-Hawthorn, Joss; Stanford, S. A. +7 more

We report deep, Keck narrowband Lyα images of the luminous z>3 radio galaxies 4C 41.17, 4C 60.07, and B2 0902+34. The images show giant, 100-200 kpc scale, emission-line nebulae, centered on these galaxies, that exhibit a wealth of morphological structure, including extended low surface brightness emission in the outer regions, radially directe…

2003 The Astrophysical Journal
eHST 139
Solar Seismic Models and the Neutrino Predictions
DOI: 10.1086/379604 Bibcode: 2003ApJ...599.1434C

Kosovichev, A. G.; Turck-Chièze, S.; Couvidat, S.

This paper focuses on the solar neutrino fluxes, the g-mode predictions, and the possible impact of the magnetic fields on the neutrino emission and transport. The Solar and Heliospheric Observatory (SOHO) spacecraft has allowed astrophysicists to achieve a major breakthrough in the knowledge of the solar core. Both GOLF and MDI instruments on SOH…

2003 The Astrophysical Journal
SOHO 139
Lyα Emission in Starbursts: Implications for Galaxies at High Redshift
DOI: 10.1086/379116 Bibcode: 2003ApJ...598..858M

Mas-Hesse, J. M.; Kunth, D.; Leitherer, C. +3 more

We present the results of a high-resolution UV two-dimensional spectroscopic survey of star-forming galaxies observed with Hubble Space Telescope Space Telescope Imaging Spectrograph. Our main aim is to map the Lyα profiles to learn about the gas kinematics and its relation with the escape of Lyα photons and to detect extended Lyα emission due to …

2003 The Astrophysical Journal
eHST 138
The Evolution of a Mass-selected Sample of Early-Type Field Galaxies
DOI: 10.1086/346206 Bibcode: 2003ApJ...587..143R

Peng, C. Y.; Keeton, C. R.; Kochanek, C. S. +7 more

We investigate the evolution of mass-selected early-type field galaxies using a sample of 28 gravitational lenses spanning the redshift range 0<~z<~1. Based on the redshift-dependent intercept of the fundamental plane in the rest-frame B band, we measure an evolution rate of dlog(M/L)B/dz=-0.56+/-0.04 (all errors are 1 σ unless no…

2003 The Astrophysical Journal
eHST 137