Aims: We study the feedback of star formation and nuclear activity on the chemistry of molecular gas in NGC 1068, a nearby (D = 14 Mpc) Seyfert 2 barred galaxy, by analyzing whether the abundances of key molecular species such as ethynyl (C2H), which is a classical tracer of photon dominated regions (PDR), change in the different environments of
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ALMA imaging of C2H emission in the disk of NGC 1068García-Burillo, S. et al.122017
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Amendment to ATel 1859: CXOM31 J004245.9+411036 is Previously Reported XMMU J004245.9+411036
The object CXOM31 J004245.9+411036, reported as a new X-ray source in ATel #1859 from M31 Chandra observations, is the previously reported XMMU J004245.9+411036 (Pietsch et al. 2008, ATel #1647). We thank W. Pietsch and M. Henze for kindly bringing this clerical error to our attention. This transient source has been observed by various space
Galache, J. L. et al.Fecha de publicación:
122008 -
An AKARI-FIS Survey of Post-AGB Stars and (Proto) Planetary Nebulae: an Analysis of Extended Emission and the Spectral Energy Distribution
We present first preliminary results from AKARI/FIS pointed observations of post-AGB stars and planetary nebulae (PNe). A first analysis of the radial (azimuthally averaged) profile of the observed sources shows no evidence for excess emission due to the presence of circumstellar dust. No (detached) circumstellar faint dust-shells are seen in the
Cox, N. et al.Fecha de publicación:
122009 -
An Atlas of Position-Velocity Diagrams in the Inner Regions of Disk Galaxies
We present an atlas of position-velocity (PV) diagrams of ionized gas in the inner regions of 23 disk galaxies. The gas kinematics have been obtained from ground-based long-slit spectra along the major axis. We discuss the variety of shapes of the emission lines in the PV diagrams that we find for the sample galaxies. To discuss the different
Funes, J. G. et al.Fecha de publicación:
122001 -
An eclipsing double-line spectroscopic binary at the stellar/substellar boundary in the Upper Scorpius OB association
Aims: We aim at constraining evolutionary models at low mass and young ages by identifying interesting transiting system members of the nearest OB association to the Sun, Upper Scorpius (USco), which has been targeted by the Kepler mission. Methods: We produced light curves for M-dwarf members of the USco region that has been surveyed during the
Lodieu, N. et al.Fecha de publicación:
122015 -
An elevation of 0.1 light-seconds for the optical jet base in an accreting Galactic black hole system
Relativistic plasma jets are observed in many systems that host accreting black holes. According to theory, coiled magnetic fields close to the black hole accelerate and collimate the plasma, leading to a jet being launched1-3. Isolating emission from this acceleration and collimation zone is key to measuring its size and understanding jet
Gandhi, P. et al.Fecha de publicación:
122017