Search Publications

HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
DOI: 10.1007/s11214-023-01019-0 Bibcode: 2023SSRv..219...74K

Verscharen, Daniel; Retinò, Alessandro; Alexandrova, Olga +47 more

HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma turbulence, a ubiquitous process occurring in the heliosphere and in plasmas throughout the universe. This will be accomplished by making simultaneous measurements at ni…

2023 Space Science Reviews
Cluster 36
PHANGS-JWST First Results: Mapping the 3.3 µm Polycyclic Aromatic Hydrocarbon Vibrational Band in Nearby Galaxies with NIRCam Medium Bands
DOI: 10.3847/2041-8213/acb0cf Bibcode: 2023ApJ...944L...7S

Sandstrom, Karin M.; Bolatto, Alberto D.; Kruijssen, J. M. Diederik +28 more

We present maps of the 3.3 µm polycyclic aromatic hydrocarbon (PAH) emission feature in NGC 628, NGC 1365, and NGC 7496 as observed with the Near-Infrared Camera imager on JWST from the PHANGS-JWST Cycle 1 Treasury project. We create maps that isolate the 3.3 µm PAH feature in the F335M filter (F335MPAH) using combinations o…

2023 The Astrophysical Journal
JWST 36
Photometric binaries, mass functions, and structural parameters of 78 Galactic open clusters
DOI: 10.1051/0004-6361/202245457 Bibcode: 2023A&A...672A..29C

Milone, Antonino P.; Vesperini, Enrico; Lagioia, Edoardo P. +8 more

Context. Binary stars play a crucial role in our understanding of the formation and evolution of star clusters and their stellar populations.
Aims: We use Gaia Data Release 3 to homogeneously analyze 78 Galactic open clusters and the unresolved binary systems they host, each composed of two main sequence (MS) stars.
Methods: We first inv…

2023 Astronomy and Astrophysics
Gaia 36
A JWST inventory of protoplanetary disk ices. The edge-on protoplanetary disk HH 48 NE, seen with the Ice Age ERS program
DOI: 10.1051/0004-6361/202347512 Bibcode: 2023A&A...679A.138S

van Dishoeck, E. F.; Pontoppidan, K. M.; Rocha, W. R. M. +24 more

Ices are the main carriers of volatiles in protoplanetary disks and are crucial to our understanding of the protoplanetary disk chemistry that ultimately sets the organic composition of planets. The Director's Discretionary-Early Release Science (DD-ERS) program Ice Age on the James Webb Space Telescope (JWST) follows the ice evolution through all…

2023 Astronomy and Astrophysics
eHST JWST 36
ELemental abundances of Planets and brown dwarfs Imaged around Stars (ELPIS). I. Potential Metal Enrichment of the Exoplanet AF Lep b and a Novel Retrieval Approach for Cloudy Self-luminous Atmospheres
DOI: 10.3847/1538-3881/acf768 Bibcode: 2023AJ....166..198Z

Fortney, Jonathan J.; Carter, Aarynn L.; Skemer, Andrew +10 more

AF Lep A+b is a remarkable planetary system hosting a gas-giant planet that has the lowest dynamical mass among directly imaged exoplanets. We present an in-depth analysis of the atmospheric composition of the star and planet to probe the planet's formation pathway. Based on new high-resolution spectroscopy of AF Lep A, we measure a uniform set of…

2023 The Astronomical Journal
Gaia 35
Observable Signature of Merging Stellar-mass Black Holes in Active Galactic Nuclei
DOI: 10.3847/1538-4357/acc4bb Bibcode: 2023ApJ...950...13T

Perna, Rosalba; Tagawa, Hiromichi; Kimura, Shigeo S. +2 more

The origin of stellar-mass black hole mergers discovered through gravitational waves is being widely debated. Mergers in the disks of active galactic nuclei (AGNs) represent a promising source of origin, with possible observational clues in the gravitational-wave data. Beyond gravitational waves, a unique signature of AGN-assisted mergers is elect…

2023 The Astrophysical Journal
INTEGRAL 35
Non-LTE radiative transfer with Turbospectrum
DOI: 10.1051/0004-6361/202243673 Bibcode: 2023A&A...669A..43G

Bergemann, Maria; Hoppe, Richard; Plez, Bertrand +4 more

Physically realistic models of stellar spectra are needed in a variety of astronomical studies, from the analysis of fundamental stellar parameters, to studies of exoplanets and stellar populations in galaxies. Here we present a new version of the widely used radiative transfer code Turbospectrum, which we update so that it is able to perform spec…

2023 Astronomy and Astrophysics
Gaia 35
Gaia Data Release 3. Hot-star radial velocities
DOI: 10.1051/0004-6361/202243685 Bibcode: 2023A&A...674A...7B

Smith, M.; Gosset, E.; Caffau, E. +38 more

Context. The second Gaia data release, DR2, contained radial velocities of stars with effective temperatures up to Teff = 6900 K. The third data release, Gaia DR3, extends this up to Teff = 14 500 K.
Aims: We derive the radial velocities for hot stars (i.e., in the Teff = 6900 − 14 500 K range) from data obtai…

2023 Astronomy and Astrophysics
Gaia 35
Hubble Space Telescope Transmission Spectroscopy for the Temperate Sub-Neptune TOI-270 d: A Possible Hydrogen-rich Atmosphere Containing Water Vapor
DOI: 10.3847/1538-3881/aca90b Bibcode: 2023AJ....165...84M

Madhusudhan, Nikku; Mikal-Evans, Thomas; Crossfield, Ian J. M. +6 more

TOI-270 d is a temperate sub-Neptune discovered by the Transiting Exoplanet Survey Satellite (TESS) around a bright (J = 9.1 mag) M3V host star. With an approximate radius of 2 R and equilibrium temperature of 350 K, TOI-270 d is one of the most promising small exoplanets for atmospheric characterization using transit spectroscopy. He…

2023 The Astronomical Journal
eHST 35
Two temperate Earth-mass planets orbiting the nearby star GJ 1002
DOI: 10.1051/0004-6361/202244991 Bibcode: 2023A&A...670A...5S

Rebolo, R.; Amado, P. J.; Caballero, J. A. +43 more

We report the discovery and characterisation of two Earth-mass planets orbiting in the habitable zone of the nearby M-dwarf GJ 1002 based on the analysis of the radial-velocity (RV) time series from the ESPRESSO and CARMENES spectrographs. The host star is the quiet M5.5 V star GJ 1002 (relatively faint in the optical, V ~ 13.8 mag, but brighter i…

2023 Astronomy and Astrophysics
Gaia 35