Search Publications

XMM-Newton observation of the Lockman Hole. I. The X-ray data
DOI: 10.1051/0004-6361:20000046 Bibcode: 2001A&A...365L..45H

Finoguenov, A.; Altieri, B.; Arnaud, M. +25 more

We report on the first deep X-ray survey with the XMM-Newton observatory during the performance verification phase. The field of the Lockman Hole, one of the best studied sky areas over a very wide range of wavelengths, has been observed. A total of ~ 100 ksec good exposure time has been accumulated. Combining the images of the European Photon Ima…

2001 Astronomy and Astrophysics
XMM-Newton 380
Far-Infrared Spectroscopy of Normal Galaxies: Physical Conditions in the Interstellar Medium
DOI: 10.1086/323046 Bibcode: 2001ApJ...561..766M

Helou, G.; Contursi, A.; Stacey, G. +10 more

The most important cooling lines of the neutral interstellar medium (ISM) lie in the far-infrared (FIR). We present measurements by the Infrared Space Observatory Long Wavelength Spectrometer of seven lines from neutral and ionized ISM of 60 normal, star-forming galaxies. The galaxy sample spans a range in properties such as morphology, FIR colors…

2001 The Astrophysical Journal
ISO 359
Quasi-Stellar Objects, Ultraluminous Infrared Galaxies, and Mergers
DOI: 10.1086/321520 Bibcode: 2001ApJ...555..719C

Stockton, Alan; Canalizo, Gabriela

We test the hypothesis that QSOs are formed via strong tidal interactions or mergers, initially going through an ultraluminous infrared phase. Our approach is to look for traces of this phase in the host galaxies of QSOs. We select a sample of low-redshift bona fide QSOs that may be in a transitionary stage between ultraluminous infrared galaxies …

2001 The Astrophysical Journal
eHST 347
X-ray spectroscopy of the cluster of galaxies Abell 1795 with XMM-Newton
DOI: 10.1051/0004-6361:20000038 Bibcode: 2001A&A...365L..87T

Kaastra, J. S.; Fabian, A. C.; Mushotzky, R. F. +8 more

The initial results from XMM-Newton observations of the rich cluster of galaxies Abell 1795 are presented. The spatially-resolved X-ray spectra taken by the European Photon Imaging Cameras (EPIC) show a temperature drop at a radius of ~ 200 kpc from the cluster center, indicating that the ICM is cooling. Both the EPIC and the Re…

2001 Astronomy and Astrophysics
XMM-Newton 347
XMM-EPIC observation of MCG-6-30-15: direct evidence for the extraction of energy from a spinning black hole?
DOI: 10.1046/j.1365-8711.2001.05066.x Bibcode: 2001MNRAS.328L..27W

Staubert, Rüdiger; Wilms, Jörn; Reynolds, Christopher S. +4 more

We present XMM-Newton European Photon Imaging Camera (EPIC) observations of the bright Seyfert 1 galaxy MCG-6-30-15, focusing on the broad Fe Kα line at ~6keV and the associated reflection continuum, which is believed to originate from the inner accretion disc. We find these reflection features to be extremely broad and redshifted, indicating an o…

2001 Monthly Notices of the Royal Astronomical Society
XMM-Newton 333
On the Nature of the Central Source in η Carinae
DOI: 10.1086/320948 Bibcode: 2001ApJ...553..837H

Davidson, K.; Hillier, D. John; Gull, T. +1 more

Long-slit spectroscopic observations of η Carinae and its Homunculus have recently been obtained using STIS on the Hubble Space Telescope (HST). We have extracted the spectrum of the central source using a 0.1"×0.13" aperture. As expected, the spectrum is very different from ground-based spectra obtained under normal seeing conditions (i.e., 1")-t…

2001 The Astrophysical Journal
eHST 332
A Correlation between Galaxy Light Concentration and Supermassive Black Hole Mass
DOI: 10.1086/338500 Bibcode: 2001ApJ...563L..11G

Graham, Alister W.; Trujillo, I.; Erwin, Peter +1 more

We present evidence for a strong correlation between the concentration of bulges and the mass of their central supermassive black hole (Mbh)-more concentrated bulges have more massive black holes. Using Cre(1/3) from Trujillo, Graham, & Caon as a measure of bulge concentration, we find that log(Mbh/M…

2001 The Astrophysical Journal
eHST 331
All-sky compiled catalogue of 2.5 million stars
Bibcode: 2001KFNT...17..409K

Kharchenko, N. V.

The all-sky Compiled Catalogue of more than 2.5 million stars with the limiting magnitude V ≈14(m) was created as a result of combining of star lists from present-day large high-precision catalogues of space (HIPPARCOS Tycho family catalogues) and ground-based (PPM, CMC11) observations and reducing them to the standard systems of corresponding ste…

2001 Kinematika i Fizika Nebesnykh Tel
Hipparcos 319
The CH out-of-plane bending modes of PAH molecules in astrophysical environments
DOI: 10.1051/0004-6361:20010242 Bibcode: 2001A&A...370.1030H

Hony, S.; Tielens, A. G. G. M.; Allamandola, L. J. +3 more

We present 10-15 mu m spectra of a sample of H ii regions, YSOs and evolved stars that show strong unidentified infrared emission features, obtained with the ISO/SWS spectrograph on-board ISO. These spectra reveal a plethora of emission features with bands at 11.0, 11.2, 12.0, 12.7, 13.5 and 14.2 mu m. These features are observed to vary considera…

2001 Astronomy and Astrophysics
ISO 315
New Insights from HST Studies of Globular Cluster Systems. I. Colors, Distances, and Specific Frequencies of 28 Elliptical Galaxies
DOI: 10.1086/321073 Bibcode: 2001AJ....121.2950K

Kundu, Arunav; Whitmore, Bradley C.

We present an analysis of the globular cluster systems of 28 elliptical galaxies using archival WFPC2 images in the V and I bands. The V-I color distributions of at least 50% of the galaxies appear to be bimodal at the present level of photometric accuracy. We argue that this is indicative of multiple epochs of cluster formation early in the histo…

2001 The Astronomical Journal
eHST 295