Search Publications

OCCASO. V. Chemical-abundance trends with Galactocentric distance and age
DOI: 10.1051/0004-6361/202347648 Bibcode: 2024A&A...687A.239C

Jordi, C.; Casamiquela, L.; Anders, F. +12 more

Context. Open clusters provide valuable information on stellar nucleosynthesis and the chemical evolution of the Galactic disk, as their age and distances can be measured more precisely with photometry than in the case of field stars.
Aims: Our aim is to study the chemical distribution of the Galactic disk using open clusters by analyzing the…

2024 Astronomy and Astrophysics
Gaia 8
VIRA: an exoplanet atmospheric retrieval framework for JWST transmission spectroscopy
DOI: 10.1093/mnras/stae633 Bibcode: 2024MNRAS.530.3252C

Madhusudhan, Nikku; Constantinou, Savvas

JWST observations are leading to important new insights into exoplanetary atmospheres through transmission spectroscopy. In order to harness the full potential of the broad spectral range and high sensitivity of JWST, atmospheric retrievals of exoplanets require a high level of robustness and accuracy in the underlying models. We present the VIRA …

2024 Monthly Notices of the Royal Astronomical Society
JWST 8
Survival in the Neptune desert: LTT 9779 b kept its atmosphere thanks to an unusually X-ray faint host star
DOI: 10.1093/mnras/stad3263 Bibcode: 2024MNRAS.527..911F

Fernández Fernández, Jorge; Wheatley, Peter J.; Jenkins, James S. +1 more

The Neptunian desert is a region in period-radius parameter space with very few Neptune-sized planets at short orbital periods. Amongst these, LTT 9779 b is the only known Neptune with a period shorter than 1 d to retain a significant H-He atmosphere. If the Neptune desert is the result of X-ray/EUV-driven photoevaporation, it is surprising that t…

2024 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 8
A hot mini-Neptune and a temperate, highly eccentric sub-Saturn around the bright K-dwarf TOI-2134
DOI: 10.1093/mnras/stad3255 Bibcode: 2024MNRAS.527.5385R

Deleuil, M.; Vanderburg, A.; Winn, J. N. +64 more

We present the characterization of an inner mini-Neptune in a 9.2292005 ± 0.0000063 d orbit and an outer mono-transiting sub-Saturn planet in a 95.50$^{+0.36}_{-0.25}$ d orbit around the moderately active, bright (mv = 8.9 mag) K5V star TOI-2134. Based on our analysis of five sectors of TESS data, we determine the radii of TOI-2134b and…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 8
A Triple Scenario for the Formation of Wide Black Hole Binaries Such as Gaia BH1
DOI: 10.3847/1538-4357/ad2356 Bibcode: 2024ApJ...964...83G

Generozov, A.; Perets, H. B.

Recently, several noninteracting black hole–stellar binaries have been identified in Gaia data—for example, Gaia BH1, where a Sun-like star is in a moderately eccentric (e = 0.44) 185 days orbit around a black hole. This orbit is difficult to explain through binary evolution. The present-day separation suggests the progenitor system would have und…

2024 The Astrophysical Journal
Gaia 8
Coronal Heating and Solar Wind Generation by Flux Cancellation Reconnection
DOI: 10.3847/1538-4357/ad03eb Bibcode: 2024ApJ...960...51P

Chitta, L. P.; Priest, E. R.; Titov, V. S. +1 more

In this paper, we propose that flux cancellation on small granular scales (≲1000 km) ubiquitously drives reconnection at a multitude of sites in the low solar atmosphere, contributing to chromospheric/coronal heating and the generation of the solar wind. We analyze the energy conversion in these small-scale flux cancellation events using both anal…

2024 The Astrophysical Journal
SolarOrbiter 8
101 eclipsing quadruple star candidates discovered in TESS full frame images
DOI: 10.1093/mnras/stad2947 Bibcode: 2024MNRAS.527.3995K

Kostov, Veselin B.; Powell, Brian P.; Rappaport, Saul A. +17 more

We present our second catalogue of quadruple star candidates, containing 101 systems discovered in TESS Full-Frame Image data. The targets were initially detected as eclipsing binary stars with the help of supervised machine learning methods applied to sectors (Sectors 1 through 54). A dedicated team of citizen scientists subsequently identified t…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 8
JWST/MIRI Detection of Suprathermal OH Rotational Emissions: Probing the Dissociation of the Water by Lyα Photons near the Protostar HOPS 370
DOI: 10.3847/2041-8213/ad3d48 Bibcode: 2024ApJ...966L..22N

Manoj, P.; Narang, Mayank; Beuther, Henrik +22 more

Using the MIRI medium-resolution spectrometer on JWST, we have detected pure rotational, suprathermal OH emissions from the vicinity of the intermediate-mass protostar HOPS 370 (OMC2/FIR3). These emissions are observed from shocked knots in a jet/outflow and originate in states of rotational quantum number as high as 46 that possess excitation ene…

2024 The Astrophysical Journal
JWST 8
Galaxy clustering at cosmic dawn from JWST/NIRCam observations to redshift z 11
DOI: 10.1093/mnras/stae2006 Bibcode: 2024MNRAS.533.2391D

Boyett, Kristan; Trenti, Michele; Leethochawalit, Nicha +1 more

We report measurements of the galaxy two-point correlation function at cosmic dawn, using photometrically selected sources from the JWST Advanced Deep Extragalactic Survey (JADES). The JWST/NIRCam data set comprises approximately $N_g \simeq 7000$ photometrically selected Lyman Break Galaxies (LBGs), spanning in the redshift range $5\le z\lt 11$. …

2024 Monthly Notices of the Royal Astronomical Society
JWST 8
Origin of the correlation between stellar kinematics and globular cluster system richness in ultradiffuse galaxies
DOI: 10.1093/mnras/stae850 Bibcode: 2024MNRAS.529.4914P

Forbes, Duncan A.; Romanowsky, Aaron J.; Brodie, Jean P. +9 more

Observational surveys have found that the dynamical masses of ultradiffuse galaxies (UDGs) correlate with the richness of their globular cluster (GC) system. This could be explained if GC-rich galaxies formed in more massive dark matter haloes. We use simulations of galaxies and their GC systems from the E-MOSAICS project to test whether the simul…

2024 Monthly Notices of the Royal Astronomical Society
eHST 8