Search Publications

XMM-Newton observations of the cluster of galaxies Abell 496. Measurements of the elemental abundances in the intracluster medium
DOI: 10.1051/0004-6361:20011317 Bibcode: 2001A&A...379..107T

Kaastra, J. S.; Molendi, S.; Ferrigno, C. +2 more

The results from XMM-Newton observations of the relaxed cluster of galaxies Abell 496 are presented. The spatially-resolved X-ray spectra taken by the European Photon Imaging Cameras show a temperature drop and a Fe abundance increase in the intra-cluster medium (ICM) towards the cD galaxy at the cluster center. The abundances of Si and S also sho…

2001 Astronomy and Astrophysics
XMM-Newton 83
The X-ray spectrum of the supernova remnant 1E 0102.2-7219
DOI: 10.1051/0004-6361:20000231 Bibcode: 2001A&A...365L.231R

Behar, E.; Kahn, S. M.; den Herder, J. W. +2 more

In this letter we present the soft X-ray (5-35 Å) spectrum of the supernova remnant (SNR) 1E 0102.2-7219 in the Small Magellanic Cloud, acquired by the reflection grating spectrometers (RGS) aboard ESA's XMM-Newton Observatory. Because the RGS features a large dispersion angle, spatial-spectral confusion is suppressed even for m…

2001 Astronomy and Astrophysics
XMM-Newton 82
Numerical simulations of weak lensing measurements
DOI: 10.1046/j.1365-8711.2001.04507.x Bibcode: 2001MNRAS.325.1065B

Refregier, Alexandre; Ellis, Richard S.; Clowe, Douglas +1 more

Weak gravitational lensing induces distortions on the images of background galaxies, and thus provides a direct measure of mass fluctuations in the Universe. The distortion signature from large-scale structure has recently been detected by several groups for the first time, opening promising prospects for the near future. Since the distortions ind…

2001 Monthly Notices of the Royal Astronomical Society
eHST 82
M Dwarfs from Hubble Space Telescope Star Counts. IV.
DOI: 10.1086/321485 Bibcode: 2001ApJ...555..393Z

Gould, Andrew; Salim, Samir; Bahcall, John N. +2 more

We study a sample of about 1400 disk M dwarfs that are found in 148 fields observed with the Wide Field Camera 2 (WFC2) on the Hubble Space Telescope and 162 fields observed with pre-repair Planetary Camera 1 (PC1), of which 95 of the WFC2 fields are newly analyzed. The method of maximum likelihood is applied to derive the luminosity function and …

2001 The Astrophysical Journal
eHST 82
Modeling the Interstellar Medium of Low Surface Brightness Galaxies: Constraining Internal Extinction, Disk Color Gradients, and Intrinsic Rotation Curve Shapes
DOI: 10.1086/318687 Bibcode: 2001ApJ...548..150M

Wood, Kenneth; Matthews, L. D.

We use a combination of three-dimensional Monte Carlo radiative transfer techniques and multiwavelength (BRHK, Hα) imaging data to investigate the nature of the interstellar medium (ISM) in the edge-on, low surface brightness (LSB) galaxy UGC 7321. Using realistic models that incorporate multiple scattering effects and clumping of the stars and th…

2001 The Astrophysical Journal
eHST 82
Global physical conditions of the interstellar medium in nearby galaxies
DOI: 10.1051/0004-6361:20010817 Bibcode: 2001A&A...375..566N

Onaka, T.; Roellig, T. L.; Negishi, T. +1 more

Far-infrared spectra (43-197 mu m) of 34 nearby galaxies obtained by the Long Wavelength Spectrometer (LWS) aboard the Infrared Space Observatory (ISO) were analyzed to investigate the general properties of interstellar matter in galaxies. The present sample includes not only normal galaxies but also starbursts and active galactic nuclei (AGNs). F…

2001 Astronomy and Astrophysics
ISO 82
Near-Infrared Imaging and [O I] Spectroscopy of IC 443 using Two Micron All Sky Survey and Infrared Space Observatory
DOI: 10.1086/318398 Bibcode: 2001ApJ...547..885R

Reach, W. T.; Rho, Jeonghee; Jarrett, T. H. +1 more

We present near-infrared J (1.25 µm), H (1.65 µm), and Ks (2.17 µm) imaging of the entire supernova remnant IC 443 from the Two Micron All Sky Survey (2MASS), and Infrared Space Observatory (ISO) LWS observations of [O I] for 11 positions in the northeast. Near-infrared emission from IC 443 was detected in all three ba…

2001 The Astrophysical Journal
ISO 82
Structural Properties of Massive Young Clusters
DOI: 10.1086/323775 Bibcode: 2001ApJ...563..151M

Maíz-Apellániz, Jesús

We have retrieved multicolor WFPC2/Hubble Space Telescope data from the STScI archive for 27 nearby massive (>~3×104 Msolar) young (<20 Myr) star clusters (MYCs). The data represents the most complete sample of clearly resolved MYCs to date. We have analyzed their structural properties and have found that they can be cl…

2001 The Astrophysical Journal
eHST 82
Hubble Space Telescope Images of Stephan's Quintet: Star Cluster Formation in a Compact Group Environment
DOI: 10.1086/321111 Bibcode: 2001AJ....122..163G

Charlton, Jane C.; Whitmore, Bradley C.; Gallagher, Sarah C. +2 more

Analysis of Hubble Space Telescope Wide Field Planetary Camera 2 images of Stephan's Quintet, Hickson Compact Group 92, yielded 115 candidate star clusters (with V-I<1.5). Unlike in merger remnants, the cluster candidates in Stephan's Quintet are not clustered in the inner regions of the galaxies; they are spread over the debris and surrounding…

2001 The Astronomical Journal
eHST 81
New Photometry for the Intermediate-Age Large Magellanic Cloud Globular Cluster NGC 2121 and the Nature of the LMC Age Gap
DOI: 10.1086/321164 Bibcode: 2001AJ....122..842R

Rich, R. Michael; Shara, Michael M.; Zurek, David

We report new photometry for the cluster NGC 2121 in the Large Magellanic Cloud, which shows a prominent hydrogen core exhaustion gap at the turnoff and a descending subgiant branch reminiscent of Galactic open clusters. We achieve an excellent fit using the Girardi isochrones, finding an age of 3.2+/-0.5 Gyr, with [Fe/H]=-0.6+/-0.2. The isochrone…

2001 The Astronomical Journal
eHST 80