Search Publications

The soft X-ray/NLR connection: a single photoionized medium?
DOI: 10.1051/0004-6361:20054091 Bibcode: 2006A&A...448..499B

Bianchi, S.; Guainazzi, M.; Chiaberge, M.

We present a sample of 8 nearby Seyfert 2 galaxies observed by HST and Chandra. All of the sources present soft X-ray emission which is coincident in extension and overall morphology with the [O iii] emission. The spectral analysis reveals that the soft X-ray emission of all the objects is likely to be dominated by a photoionized gas. This is stro…

2006 Astronomy and Astrophysics
XMM-Newton eHST 218
X-ray spectral survey with XMM-Newton of a complete sample of nearby Seyfert galaxies
DOI: 10.1051/0004-6361:20053893 Bibcode: 2006A&A...446..459C

Cappi, M.; Filippenko, A. V.; Piconcelli, E. +15 more

Results obtained from an X-ray spectral survey of nearby Seyfert galaxies using XMM-Newton are reported. The sample was optically selected, well defined, complete in B magnitude, and distance limited: it consists of the nearest (D ⪉22 Mpc) 27 Seyfert galaxies (9 of type 1, 18 of type 2) taken from the Ho et al. (1997a, ApJS, 112, 315) sample. This…

2006 Astronomy and Astrophysics
XMM-Newton 214
2MASS wide field extinction maps. I. The Pipe nebula
DOI: 10.1051/0004-6361:20042474 Bibcode: 2006A&A...454..781L

Alves, J.; Lombardi, M.; Lada, C. J.

Context: .
Aims: . We present a 8°×6°, high resolution extinction map of the Pipe nebula using 4.5 million stars from the Two Micron All Sky Survey (2MASS) point source catalog.
Methods: . The use of Nicer (Lombardi & Alves 2001, A&A, 377, 1023), a robust and optimal technique to map the dust column density, allows us to detect a…

2006 Astronomy and Astrophysics
Hipparcos 213
Keplerian discs around post-AGB stars: a common phenomenon?
DOI: 10.1051/0004-6361:20054062 Bibcode: 2006A&A...448..641D

Waters, L. B. F. M.; Dejonghe, H.; de Ruyter, S. +3 more

Aims.We aim at showing that the broad-band SED characteristics of our sample of post-AGB stars are best interpreted, assuming the circumstellar dust is stored in Keplerian rotating passive discs.Methods.We present a homogeneous and systematic study of the Spectral Energy Distributions (SEDs) of a sample of 51 post-AGB objects. The selection criter…

2006 Astronomy and Astrophysics
IUE 204
Evolutionary state of magnetic chemically peculiar stars
DOI: 10.1051/0004-6361:20054596 Bibcode: 2006A&A...450..763K

Kochukhov, O.; Bagnulo, S.

Context: .The photospheres of about 5-10% of the upper main sequence stars exhibit remarkable chemical anomalies. Many of these chemically peculiar (CP) stars have a global magnetic field, the origin of which is still a matter of debate.
Aims: .We present a comprehensive statistical investigation of the evolution of magnetic CP stars, aimed at…

2006 Astronomy and Astrophysics
Hipparcos 204
Spectral analysis of the Galactic e+e- annihilation emission
DOI: 10.1051/0004-6361:20053765 Bibcode: 2006A&A...445..579J

Knödlseder, J.; Marcowith, A.; Guessoum, N. +5 more

We present a spectral analysis of the e+e- annihilation emission from the Galactic Centre region based on the first year of measurements made with the spectrometer SPI of the INTEGRAL mission. We have found that the annihilation spectrum can be modelled by the sum of a narrow and a broad 511 keV line plus an ortho-positronium…

2006 Astronomy and Astrophysics
INTEGRAL 199
Effective temperature scale and bolometric corrections from 2MASS photometry
DOI: 10.1051/0004-6361:20054021 Bibcode: 2006A&A...450..735M

Ribas, I.; Jordi, C.; Masana, E.

We present a method to determine effective temperatures, angular semi-diameters and bolometric corrections for population I and II FGK type stars based on V and 2MASS IR photometry. Accurate calibration is accomplished by using a sample of solar analogues, whose average temperature is assumed to be equal to the solar effective temperature of 5777 …

2006 Astronomy and Astrophysics
Hipparcos 198
The great observatories origins deep survey. VLT/FORS2 spectroscopy in the GOODS-South Field: Part II
DOI: 10.1051/0004-6361:20054796 Bibcode: 2006A&A...454..423V

Popesso, P.; Cesarsky, C.; Stern, D. +16 more

Aims.We present the second campaign of the ESO/GOODS program of spectroscopy of faint galaxies in the GOODS-South field.
Methods: .Objects were selected as candidates for VLT/FORS2 observations primarily based on the expectation that the detection and measurement of their spectral features would benefit from the high throughput and spectral re…

2006 Astronomy and Astrophysics
eHST 195
Origin of the Galactic ridge X-ray emission
DOI: 10.1051/0004-6361:20054268 Bibcode: 2006A&A...452..169R

Sunyaev, R.; Revnivtsev, M.; Sazonov, S. +2 more

We analyze a map of the Galactic ridge X-ray emission (GRXE) constructed in the 3-20 keV energy band from RXTE/PCA scan and slew observations. We show that the GRXE intensity follows the Galactic near-infrared surface brightness closely and thus traces the Galactic stellar mass distribution. The GRXE consists of two spatial components that can be …

2006 Astronomy and Astrophysics
INTEGRAL 187
The unprecedented optical outburst of the quasar 3C 454.3. The WEBT campaign of 2004-2005
DOI: 10.1051/0004-6361:20064817 Bibcode: 2006A&A...453..817V

Lee, C. -U.; Lähteenmäki, A.; Umana, G. +85 more

Context: .The radio quasar 3C 454.3 underwent an exceptional optical outburst lasting more than 1 year and culminating in spring 2005. The maximum brightness detected was R=12.0, which represents the most luminous quasar state thus far observed (MB ∼ -31.4).
Aims: .In order to follow the emission behaviour of the …

2006 Astronomy and Astrophysics
INTEGRAL 178