Search Publications

The impact of stellar feedback from velocity-dependent ionized gas maps - a MUSE view of Haro 11
DOI: 10.1093/mnras/stz1414 Bibcode: 2019MNRAS.487.3183M

Östlin, G.; Hayes, M.; Adamo, A. +6 more

We have used the capability of the Multi-Unit Spectroscopic Explorer (MUSE) instrument to explore the impact of stellar feedback at large scales in Haro 11, a galaxy under extreme starburst condition and one of the first galaxies where Lyman continuum (LyC) has been detected. Using H α, [O III] λ5007, and [O I] λ6300 emission lines from deep MUSE …

2019 Monthly Notices of the Royal Astronomical Society
eHST 35
NuSTAR and XMM-Newton broad-band spectrum of SAX J1808.4-3658 during its latest outburst in 2015
DOI: 10.1093/mnras/sty2974 Bibcode: 2019MNRAS.483..767D

Sanna, A.; Papitto, A.; Di Salvo, T. +4 more

The first discovered accreting millisecond pulsar, SAX J1808.4-3658, went into X-ray outburst in 2015 April. We triggered a 100 ks XMM-Newton ToO, taken at the peak of the outburst, and a 55 ks NuSTAR ToO, performed 4 d apart. We report here the results of a detailed spectral analysis of both the XMM-Newton and NuSTAR spectra. While the XMM-Newton…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 35
Faint end of the z ∼ 3-7 luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE
DOI: 10.1051/0004-6361/201834471 Bibcode: 2019A&A...628A...3D

Laporte, N.; Bauer, F. E.; Bina, D. +21 more

Contact. This paper presents the results obtained with the Multi-Unit Spectroscopic Explorer (MUSE) at the ESO Very Large Telescope on the faint end of the Lyman-alpha luminosity function (LF) based on deep observations of four lensing clusters. The goal of our project is to set strong constraints on the relative contribution of the Lyman-alpha em…

2019 Astronomy and Astrophysics
eHST 35
The Red Dead Redemption Survey of Circumgalactic Gas about Massive Galaxies. I. Mass and Metallicity of the Cool Phase
DOI: 10.3847/1538-4357/ab378e Bibcode: 2019ApJ...883....5B

Bowen, David V.; Tejos, Nicolas; Lehner, Nicolas +6 more

We present a search for H I in the circumgalactic medium (CGM) of 21 massive (< {log}{M}\star > ∼ 11.4), luminous red galaxies (LRGs) at z ∼ 0.5. Using UV spectroscopy of QSO sightlines projected within 500 kpc (∼{R}vir}) of these galaxies, we detect H I absorption in 11/21 sightlines, including two partial Lyman limit …

2019 The Astrophysical Journal
eHST 35
Photochemistry of water in the martian thermosphere and its effect on hydrogen escape
DOI: 10.1016/j.icarus.2018.10.033 Bibcode: 2019Icar..321...62K

Krasnopolsky, Vladimir A.

Recent SPICAM IR solar occultations reveal significant abundances of water vapor up to ≈80 km near Mars perihelion. These abundances are stimulated by dust that heats the atmosphere and precludes condensation of water. This phenomenon correlates with detections of high escape of hydrogen near perihelion using the H Lyman-alpha in the SPICAM UV and…

2019 Icarus
MEx eHST 35
Multiple stellar populations in NGC 1866. New clues from Cepheids and colour-magnitude diagram
DOI: 10.1051/0004-6361/201936409 Bibcode: 2019A&A...631A.128C

Girardi, Léo; Marigo, Paola; Goudfrooij, Paul +5 more

We performed a comprehensive study of the stellar populations in the young Large Magellanic Cloud cluster NGC 1866, combining the analysis of its best-studied Cepheids with that of a very accurate colour-magnitude diagram (CMD) obtained from the most recent Hubble Space Telescope photometry. We used a Bayesian method based on new PARSEC stellar ev…

2019 Astronomy and Astrophysics
eHST 35
Extreme Debris Disk Variability: Exploring the Diverse Outcomes of Large Asteroid Impacts During the Era of Terrestrial Planet Formation
DOI: 10.3847/1538-3881/ab1260 Bibcode: 2019AJ....157..202S

Reichart, D. E.; Rujopakarn, W.; Dong, Ruobing +14 more

The most dramatic phases of terrestrial planet formation are thought to be oligarchic and chaotic growth, on timescales of up to 100-200 Myr, when violent impacts occur between large planetesimals of sizes up to protoplanets. Such events are marked by the production of large amounts of debris, as has been observed in some exceptionally bright and …

2019 The Astronomical Journal
Gaia 35
Speckle Interferometry at SOAR in 2018
DOI: 10.3847/1538-3881/ab24e4 Bibcode: 2019AJ....158...48T

Tokovinin, Andrei; Briceño, Cesar; Horch, Elliott P. +2 more

The results of speckle interferometric observations at the 4.1 m Southern Astrophysical Research Telescope (SOAR) in 2018 are given, totaling 3097 measurements of 2427 resolved pairs with separations from 11 mas to 5.″9 (median 0.″15, magnitude difference up to 7 mag) and nonresolutions of 624 targets. This work continues our long-term speckle pro…

2019 The Astronomical Journal
Gaia Hipparcos 35
A LOFAR-IRAS cross-match study: the far-infrared radio correlation and the 150 MHz luminosity as a star-formation rate tracer
DOI: 10.1051/0004-6361/201935913 Bibcode: 2019A&A...631A.109W

Prandoni, I.; Wang, L.; Shimwell, T. W. +15 more


Aims: We aim to study the far-infrared radio correlation (FIRC) at 150 MHz in the local Universe (at a median redshift ⟨z⟩∼0.05) and improve the use of the rest-frame 150 MHz luminosity, L150, as a star-formation rate (SFR) tracer, which is unaffected by dust extinction.
Methods: We cross-match the 60 µm selected Revised…

2019 Astronomy and Astrophysics
AKARI 35
Empirical Modeling of CME Evolution Constrained to ACE/SWICS Charge State Distributions
DOI: 10.3847/1538-4357/ab0e11 Bibcode: 2019ApJ...874..164R

Landi, Enrico; Rivera, Yeimy J.; Lepri, Susan T. +1 more

It is generally accepted that coronal mass ejections (CMEs) undergo rapid heating as they are released from the Sun. However, to date, the heating mechanism remains an open question. To gain insight into the plasma heating, we derive the density, temperature, and velocity evolution of the 2005 January 9 interplanetary CME event from launch to ion …

2019 The Astrophysical Journal
SOHO 35