Search Publications

Smashing the Guitar: An Evolving Neutron Star Bow Shock
DOI: 10.1086/381498 Bibcode: 2004ApJ...600L..51C

Chatterjee, S.; Cordes, J. M.

The Guitar Nebula is a spectacular example of an Hα bow shock nebula produced by the interaction of a neutron star with its environment. The radio pulsar B2224+65 is traveling at ~800-1600 km s-1 (for a distance of 1-2 kpc), placing it on the high-velocity tail of the pulsar velocity distribution. Here we report time evolution in the sh…

2004 The Astrophysical Journal
eHST 62
Truncation of stellar disks in galaxies at z ≈ 1
DOI: 10.1051/0004-6361:200400090 Bibcode: 2004A&A...427L..17P

Pérez, I.

We report here the first evidence for stellar disk truncation at high redshift, based on surface photometry of a sample of 16 high redshift (0.6<z<1.0) disk galaxies from the GOODS HST/ACS data. The radial profiles are best fit by a double exponential profile. This result agrees with the profile of disks in local galaxies. The cosmological s…

2004 Astronomy and Astrophysics
eHST 61
A Hubble Space Telescope WFPC2 Investigation of the Disk-Halo Interface in NGC 891
DOI: 10.1086/422489 Bibcode: 2004AJ....128..674R

Norman, Colin A.; Dettmar, Ralf-Jürgen; Rossa, Jörn +1 more

We present deep narrowband observations with high spatial resolution of extraplanar diffuse ionized gas in the halo of NGC 891, obtained with the WFPC2 on board the HST. Our Hα observations, centered on the northern part of NGC 891, reveal an extended gaseous halo, which fills almost the entire field of view of our WFPC2 observation. Whereas NGC 8…

2004 The Astronomical Journal
eHST 61
Discovery of X-ray absorption features from the dipping low-mass X-ray binary XB 1916-053 with XMM-Newton
DOI: 10.1051/0004-6361:20034550 Bibcode: 2004A&A...418.1061B

Parmar, A. N.; Boirin, L.; Paltani, S. +2 more

We report the discovery of narrow Fe XXV and Fe XXVI Kα X-ray absorption lines at 6.65+0.05-0.02 and 6.95+0.05-0.04 keV in the persistent emission of the dipping low-mass X-ray binary (LMXB) XB 1916-053 during an XMM-Newton observation performed in September 2002. In addition, there is marginal evidence …

2004 Astronomy and Astrophysics
XMM-Newton 61
The Hubble Deep Field North SCUBA Super-map - II. Multiwavelength properties
DOI: 10.1111/j.1365-2966.2004.08335.x Bibcode: 2004MNRAS.355..485B

Nandra, Kirpal; Halpern, Mark; Chapman, Scott +3 more

We present radio, optical and X-ray-detected counterparts to the submillimetre sources found using SCUBA in the Hubble Deep Field North region (GOODS-N). A new counterpart identification statistic is developed to identify properties of galaxies detected at other wavelengths that can be used to aid counterpart identification. We discriminate betwee…

2004 Monthly Notices of the Royal Astronomical Society
ISO 61
On the network structures in solar equatorial coronal holes. Observations of SUMER and MDI on SOHO
DOI: 10.1051/0004-6361:20047027 Bibcode: 2004A&A...424.1025X

Wilhelm, K.; Marsch, E.; Xia, L. D.

By combining observations of the Sun made by SUMER and MDI aboard SOHO, the network structures in equatorial coronal holes have been studied, in particular the relationship between the ultraviolet emission-line parameters (line radiance, Doppler shift and line width) and the underlying magnetic field. The bases of coronal holes seen in chromospher…

2004 Astronomy and Astrophysics
SOHO 61
First observation of Jupiter by XMM-Newton
DOI: 10.1051/0004-6361:20041149 Bibcode: 2004A&A...424..331B

Branduardi-Raymont, G.; Soria, R.; Ramsay, G. +4 more

We present the first X-ray observation of Jupiter by XMM-Newton. Images taken with the EPIC cameras show prominent emission, essentially all confined to the 0.2-2.0 keV band, from the planet's auroral spots; their spectra can be modelled with a combination of unresolved emission lines of highly ionised oxygen (OVII and OVIII), and a pseudo-continu…

2004 Astronomy and Astrophysics
XMM-Newton 61
Organic matter in Seyfert 2 nuclei: Comparison with our Galactic center lines of sight
DOI: 10.1051/0004-6361:20047067 Bibcode: 2004A&A...423..549D

Dartois, E.; d'Hendecourt, L.; Marco, O. +3 more

We present ESO - Very Large Telescope and ESA - Infrared Space Observatory 3 to 4 µm spectra of Seyfert 2 nuclei as compared to our galactic center lines of sight. The diffuse interstellar medium probed in both environments displays the characteristic 3.4 µm aliphatic CH stretch absorptions of refractory carbonaceous material. The prof…

2004 Astronomy and Astrophysics
ISO 61
About the rotation of the solar radiative interior
DOI: 10.1023/B:SOLA.0000031395.90891.ce Bibcode: 2004SoPh..220..269G

Henney, C. J.; Howe, R.; Eff-Darwich, A. +13 more

In the modern era of helioseismology we have a wealth of high-quality data available, e.g., more than 6 years of data collected by the various instruments on board the SOHO mission, and an even more extensive ground-based set of observations covering a full solar cycle. Thanks to this effort a detailed picture of the internal rotation of the Sun h…

2004 Solar Physics
SOHO 61
Abundance analysis of targets for the COROT/MONS asteroseismology missions. II. Abundance analysis of the COROT main targets
DOI: 10.1051/0004-6361:20040464 Bibcode: 2004A&A...425..683B

Magain, P.; Catala, C.; Bikmaev, I. F. +13 more

One of the goals of the ground-based support program for the COROT and MONS/RÖMER satellite missions is to characterize suitable target stars for the part of the missions dedicated to asteroseismology. We present the detailed abundance analysis of nine of the potential COROT main targets using the semi-automatic software VWA. For two additional CO…

2004 Astronomy and Astrophysics
Hipparcos 61