Search Publications

The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). VIII. Diffuse dust in the Virgo intra-cluster space
DOI: 10.1051/0004-6361/201937024 Bibcode: 2020A&A...633L...7L

Andreani, P.; Bianchi, S.; Boselli, A. +5 more


Aims: We present the first detection of diffuse dust in the intra-cluster medium of the Virgo cluster out to ∼0.4 virial radii, and study the radial variation of its properties on a radial scale of the virial radius.
Methods: Analysing near-UV - i colours for a sample of ∼12 000 background galaxies with redshifts 0.02 < z < 0.8, we…

2020 Astronomy and Astrophysics
Herschel 10
The Gaia-ESO Survey: Spectroscopic-asteroseismic analysis of K2 stars in Gaia-ESO. The K2 Galactic Caps Project
DOI: 10.1051/0004-6361/201936726 Bibcode: 2020A&A...643A..83W

Gilmore, G.; Bayo, A.; Lardo, C. +33 more

Context. The extensive stellar spectroscopic datasets that are available for studies in Galactic Archeaology thanks to, for example, the Gaia-ESO Survey, now benefit from having a significant number of targets that overlap with asteroseismology projects such as Kepler, K2, and CoRoT. Combining the measurements from spectroscopy and asteroseismolog…

2020 Astronomy and Astrophysics
Gaia 10
The giant outburst of 4U 0115+634 in 2011 with Suzaku and RXTE. Minimizing cyclotron line biases
DOI: 10.1051/0004-6361/201935666 Bibcode: 2020A&A...634A..99B

Rothschild, Richard E.; Fürst, Felix; Grinberg, Victoria +19 more

We present an analysis of X-ray spectra of the high-mass X-ray binary 4U 0115+634 as observed with Suzaku and RXTE in 2011 July, during the fading phase of a giant X-ray outburst. We used a continuum model consisting of an absorbed cutoff power law and an ad hoc Gaussian emission feature centered around 8.5 keV, which we attribute to cyclotron emi…

2020 Astronomy and Astrophysics
Gaia 10
KELT-17: a chemically peculiar Am star and a hot-Jupiter planet
DOI: 10.1051/0004-6361/202038843 Bibcode: 2020A&A...641A.145S

González, J. F.; Jofré, E.; Jaque Arancibia, M. +6 more

Context. There is very little information to be found in the literature regarding the detection of planets orbiting chemically peculiar stars.
Aims: Our aim is to determine the detailed chemical composition of the remarkable planet host star KELT-17. This object hosts a hot-Jupiter planet with 1.31 MJup detected by transits, and it…

2020 Astronomy and Astrophysics
Gaia 10
Neglected X-ray discovered polars. II. The peculiar eclipsing binary HY Eridani
DOI: 10.1051/0004-6361/201936626 Bibcode: 2020A&A...634A..91B

Burwitz, V.; Beuermann, K.; Schwope, A. +2 more

We report on the X-ray observations of the eclipsing polar HY Eri (RX J0501-0359), along with its photometric, spectrophotometric, and spectropolarimetric optical variations, collected over 30 years. With an orbital period of 2.855 h, HY Eri falls near the upper edge of the 2-3 h period gap. After 2011, the system went into a pr…

2020 Astronomy and Astrophysics
Gaia XMM-Newton 10
APEX CO observations towards the photodissociation region of RCW 120
DOI: 10.1051/0004-6361/202037713 Bibcode: 2020A&A...639A..93F

Zavagno, A.; Russeil, D.; Schuller, F. +3 more

Context. The edges of ionized (H II) regions are important sites for the formation of (high-mass) stars. Indeed, at least 30% of the Galactic high-mass-star formation is observed there. The radiative and compressive impact of the H II region could induce star formation at the border following different mechanisms such as the collect and collapse o…

2020 Astronomy and Astrophysics
Herschel 10
A high redshift population of galaxies at the North Ecliptic Pole. Unveiling the main sequence of dusty galaxies
DOI: 10.1051/0004-6361/202037838 Bibcode: 2020A&A...641A.129B

Valtchanov, I.; White, G. J.; Małek, K. +16 more

Context. Dusty high-z galaxies are extreme objects with high star formation rates (SFRs) and luminosities. Characterising the properties of this population and analysing their evolution over cosmic time is key to understanding galaxy evolution in the early Universe.
Aims: We select a sample of high-z dusty star-forming galaxies (DSFGs) and ev…

2020 Astronomy and Astrophysics
AKARI Herschel 10
The molecular mass function of the local Universe
DOI: 10.1051/0004-6361/202038675 Bibcode: 2020A&A...643L..11A

Andreani, P.; Boselli, A.; Vio, R. +4 more


Aims: We construct the molecular mass function using the bivariate K-band-mass function (BMF) of the Herschel Reference Survey (HRS), which is a volume-limited sample that has already been widely studied at the entire electromagnetic spectrum.
Methods: The molecular mass function was derived from the K-band and the gas mass cumulative di…

2020 Astronomy and Astrophysics
Herschel 10
Doppler shift oscillations of a sunspot detected by CYRA and IRIS
DOI: 10.1051/0004-6361/202039007 Bibcode: 2020A&A...642A.231L

Li, D.; Su, J. T.; Cao, W. +4 more

Context. The carbon monoxide (CO) molecular line at around 46655 Å in solar infrared spectra is often used to investigate the dynamic behavior of the cold heart of the solar atmosphere, i.e., sunspot oscillation, especially at the sunspot umbra.
Aims: We investigated sunspot oscillation at Doppler velocities of the CO 7-6 R67 and 3-2 R14 line…

2020 Astronomy and Astrophysics
IRIS 10
NuSTAR observation of the supergiant fast X-ray transient IGR J11215-5952 during its 2017 outburst
DOI: 10.1051/0004-6361/202038078 Bibcode: 2020A&A...638A..71S

Tiengo, A.; Sidoli, L.; Esposito, P. +4 more

We report on the results of a NuSTAR observation of the supergiant fast X-ray transient pulsar IGR J11215-5952 during the peak of its outburst in June 2017. IGR J11215-5952 is the only SFXT undergoing strictly periodic outbursts (every 165 days). NuSTAR caught several X-ray flares, spanning a dynamic range of 100, and detected X-ray pulsations at …

2020 Astronomy and Astrophysics
Gaia 10