Search Publications

A matched filter approach for blind joint detection of galaxy clusters in X-ray and SZ surveys
DOI: 10.1051/0004-6361/201731984 Bibcode: 2018A&A...614A..82T

Arnaud, M.; Melin, J. -B.; Tarrío, P.

The combination of X-ray and Sunyaev-Zeldovich (SZ) observations can potentially improve the cluster detection efficiency, when compared to using only one of these probes, since both probe the same medium, the hot ionized gas of the intra-cluster medium. We present a method based on matched multifrequency filters (MMF) for detecting galaxy cluster…

2018 Astronomy and Astrophysics
Planck XMM-Newton 12
Heating of the solar photosphere during a white-light flare
DOI: 10.1051/0004-6361/201833946 Bibcode: 2018A&A...620A.183J

Kleint, Lucia; Kašparová, Jana; Jurčák, Jan +1 more

Context. The Fe I lines observed by the Hinode/SOT spectropolarimeter were always seen in absorption, apart from the extreme solar limb. Here we analyse a unique dataset capturing these lines in emission during a solar white-light flare.
Aims: We analyse the temperature stratification in the solar photosphere during a white-light flare and co…

2018 Astronomy and Astrophysics
Hinode 12
Variability of extragalactic sources: its contribution to the link between ICRF and the future Gaia Celestial Reference Frame
DOI: 10.1051/0004-6361/201731362 Bibcode: 2018A&A...611A..52T

Souchay, J.; Taris, F.; Andrei, A. +3 more

Context. The first release of the Gaia catalog is available since 14 September 2016. It is a first step in the realization of the future Gaia reference frame. This reference frame will be materialized by the optical positions of the sources and will be compared with and linked to the International Celestial Reference Frame, materialized by the rad…

2018 Astronomy and Astrophysics
Gaia 12
The triple system HD 150136: From periastron passage to actual masses
DOI: 10.1051/0004-6361/201832810 Bibcode: 2018A&A...616A..75M

Gosset, E.; Manfroid, J.; Sana, H. +6 more

Context. The triple system HD 150136 is composed of an O3 V((f*))-O3.5 V((f+)) primary, of an O5.5-6 V((f)) secondary, and of a more distant O6.5-7 V((f)) tertiary. The latter component went through periastron in 2015-2016, an event that will not occur again within the next eight years.
Aims: We aim to analyse the tertia…

2018 Astronomy and Astrophysics
Gaia 12
FUV line emission, gas kinematics, and discovery of [Fe XXI] λ1354.1 in the sightline toward a filament in M87
DOI: 10.1051/0004-6361/201732510 Bibcode: 2018A&A...617A.123A

Anderson, Michael E.; Sunyaev, Rashid

We present new Hubble Space Telescope - Cosmic Origins Spectrograph (HST-COS) G130M spectroscopy which we have obtained for a sightline toward a filament projected 1.9 kpc from the nucleus of M87, near the edge of the inner radio lobe to the east of the nucleus. The combination of the sensitivity of COS and the proximity of M87 allows us to study …

2018 Astronomy and Astrophysics
Herschel eHST 12
CXOU J160103.1-513353: another central compact object with a carbon atmosphere?
DOI: 10.1051/0004-6361/201833271 Bibcode: 2018A&A...618A..76D

Santangelo, A.; Doroshenko, V.; Suleimanov, V.

We report on the analysis of XMM-Newton observations of the central compact object CXOU J160103.1-513353 located in the center of the non-thermally emitting supernova remnant (SNR) G330.2+1.0. The X-ray spectrum of the source is well described with either single-component carbon or two-component hydrogen atmosphere models. In the latter case, the …

2018 Astronomy and Astrophysics
XMM-Newton 12
The local rotation curve of the Milky Way based on SEGUE and RAVE data
DOI: 10.1051/0004-6361/201731143 Bibcode: 2018A&A...614A..63S

Watson, F.; Munari, U.; Steinmetz, M. +13 more


Aims: We construct the rotation curve of the Milky Way in the extended solar neighbourhood using a sample of Sloan Extension for Galactic Understanding and Exploration (SEGUE) G-dwarfs. We investigate the rotation curve shape for the presence of any peculiarities just outside the solar radius as has been reported by some authors.
Methods…

2018 Astronomy and Astrophysics
Gaia 12
Super lithium-rich K giant with low 12C to 13C ratio
DOI: 10.1051/0004-6361/201730389 Bibcode: 2018A&A...615A..74Z

Zhao, G.; Pan, K.; Gao, Q. +5 more

Context. The lithium abundances in a few percent of giants exceed the value predicted by the standard stellar evolution models, and the mechanisms of Li enhancement are still under debate. The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) survey has obtained over six million spectra in the past five years, and thus provides a …

2018 Astronomy and Astrophysics
Gaia 12
Ratio of black hole to galaxy mass of an extremely red dust-obscured galaxy at z = 2.52
DOI: 10.1051/0004-6361/201833943 Bibcode: 2018A&A...620L...3M

Marconi, A.; Iwasawa, K.; Wang, W. -H. +7 more

We present a near-infrared (NIR) spectrum of WISE J104222.11+164115.3, an extremely red dust-obscured galaxy (DOG), which has been observed with the Long-slit Intermediate Resolution Infrared Spectrograph (LIRIS) on the 4.2m William Hershel Telescope. This object was selected as a hyper-luminous DOG candidate at z ∼ 2 by combining the optical and …

2018 Astronomy and Astrophysics
AKARI 11
Chromospheric counterparts of solar transition region unresolved fine structure loops
DOI: 10.1051/0004-6361/201832762 Bibcode: 2018A&A...611L...6P

De Pontieu, Bart; Hansteen, Viggo H.; Rouppe van der Voort, Luc +1 more

Low-lying loops have been discovered at the solar limb in transition region temperatures by the Interface Region Imaging Spectrograph (IRIS). They do not appear to reach coronal temperatures, and it has been suggested that they are the long-predicted unresolved fine structures (UFS). These loops are dynamic and believed to be visible during both h…

2018 Astronomy and Astrophysics
IRIS 11