Search Publications

A likely flyby of binary protostar Z CMa caught in action
DOI: 10.1038/s41550-021-01558-y Bibcode: 2022NatAs...6..331D

Henning, Thomas; Dong, Ruobing; Pyo, Tae-Soo +16 more

Close encounters between young stellar objects in star-forming clusters are expected to markedly perturb circumstellar disks. Such events are witnessed in numerical simulations of star formation1-3, but few direct observations of ongoing encounters have been made. Here we report sub-0.1″-resolution Atacama Large Millimeter/Submillimeter…

2022 Nature Astronomy
Gaia 34
Systematic KMTNet planetary anomaly search. V. Complete sample of 2018 prime-field
DOI: 10.1051/0004-6361/202243744 Bibcode: 2022A&A...664A..13G

Stassun, Keivan G.; Han, Cheongho; Udalski, Andrzej +69 more

We complete the analysis of all 2018 prime-field microlensing planets identified by the Korea Microlensing Telescope Network (KMTNet) Anomaly Finder. Among the ten previously unpublished events with clear planetary solutions, eight are either unambiguously planetary or are very likely to be planetary in nature: OGLE-2018-BLG-1126, KMT-2018-BLG-200…

2022 Astronomy and Astrophysics
Gaia eHST 34
Tracing the Milky Way warp and spiral arms with classical Cepheids
DOI: 10.1051/0004-6361/202243273 Bibcode: 2022A&A...668A..40L

Kovtyukh, V.; Lemasle, B.; Kniazev, A. +10 more

Context. Mapping the Galactic spiral structure is a difficult task since the Sun is located in the Galactic plane and because of dust extinction. For these reasons, molecular masers in radio wavelengths have been used with great success to trace the Milky Way spiral arms. Recently, Gaia parallaxes have helped in investigating the spiral structure …

2022 Astronomy and Astrophysics
Gaia 34
Intermediate- and high-velocity clouds in the Milky Way - I. Covering factors and vertical heights
DOI: 10.1093/mnras/stac987 Bibcode: 2022MNRAS.513.3228L

Lehner, Nicolas; Howk, J. Christopher; Marasco, Antonino +1 more

Intermediate- and high-velocity clouds (IVCs, HVCs) are a potential source of fuel for star formation in the Milky Way (MW), but their origins and fates depend sensitively on their distances. We search for IVCs and HVCs in HST high-resolution ultraviolet spectra of 55 halo stars at vertical heights $|z|\gtrsim \,1$ kpc. We show that IVCs (40 ≤ |$v…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 34
Retrieving the C and O Abundances of HR 7672 AB: A Solar-type Primary Star with a Benchmark Brown Dwarf
DOI: 10.3847/1538-3881/ac56e2 Bibcode: 2022AJ....163..189W

Fitzgerald, Michael P.; Skemer, Andrew; Wallack, Nicole L. +30 more

A benchmark brown dwarf (BD) is a BD whose properties (e.g., mass and chemical composition) are precisely and independently measured. Benchmark BDs are valuable in testing theoretical evolutionary tracks, spectral synthesis, and atmospheric retrievals for substellar objects. Here, we report results of atmospheric retrieval on a synthetic spectrum …

2022 The Astronomical Journal
Gaia 34
Asymmetrical tidal tails of open star clusters: stars crossing their cluster's práh challenge Newtonian gravitation
DOI: 10.1093/mnras/stac2563 Bibcode: 2022MNRAS.517.3613K

Famaey, Benoit; Kroupa, Pavel; Boffin, Henri M. J. +14 more

After their birth a significant fraction of all stars pass through the tidal threshold (práh) of their cluster of origin into the classical tidal tails. The asymmetry between the number of stars in the leading and trailing tails tests gravitational theory. All five open clusters with tail data (Hyades, Praesepe, Coma Berenices, COIN-Gaia 13, NGC 7…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 34
METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble Program. III. Interstellar Depletions, Dust-to-Metal, and Dust-to-Gas Ratios versus Metallicity
DOI: 10.3847/1538-4357/ac5248 Bibcode: 2022ApJ...928...90R

Jenkins, Edward B.; Yanchulova Merica-Jones, Petia; Gordon, Karl D. +9 more

The metallicity and gas density dependence of interstellar depletions, the dust-to-gas (D/G), and dust-to-metal (D/M) ratios have important implications for how accurately we can trace the chemical enrichment of the universe, either by using FIR dust emission as a tracer of the ISM or by using spectroscopy of damped Lyα systems to measure chemical…

2022 The Astrophysical Journal
eHST 34
The mass and size of Herbig disks as seen by ALMA
DOI: 10.1051/0004-6361/202142164 Bibcode: 2022A&A...658A.112S

van Dishoeck, E. F.; Hogerheijde, M. R.; Stapper, L. M. +1 more

Context. Many population studies have been performed over the past decade with the Atacama Large millimeter/submillimeter Array (ALMA) to understand the bulk properties of protoplanetary disks around young stars. The studied populations have mostly consisted of late spectral type (i.e., G, K & M) stars, with relatively few more massive Herbig …

2022 Astronomy and Astrophysics
Gaia 34
A Possible Alignment Between the Orbits of Planetary Systems and their Visual Binary Companions
DOI: 10.3847/1538-3881/ac517f Bibcode: 2022AJ....163..207C

Vanderburg, Andrew; Bieryla, Allyson; Latham, David W. +111 more

Astronomers do not have a complete picture of the effects of wide-binary companions (semimajor axes greater than 100 au) on the formation and evolution of exoplanets. We investigate these effects using new data from Gaia Early Data Release 3 and the Transiting Exoplanet Survey Satellite mission to characterize wide-binary systems with transiting e…

2022 The Astronomical Journal
Gaia 34
Clearing the Hurdle: The Mass of Globular Cluster Systems as a Function of Host Galaxy Mass
DOI: 10.3847/1538-4357/ac33b0 Bibcode: 2022ApJ...926..162E

Harris, William E.; Eadie, Gwendolyn M.; Springford, Aaron

Current observational evidence suggests that all large galaxies contain globular clusters (GCs), while the smallest galaxies do not. Over what galaxy mass range does the transition from GCs to no GCs occur? We investigate this question using galaxies in the Local Group (LG), nearby dwarf galaxies, and galaxies in the Virgo Cluster Survey. We consi…

2022 The Astrophysical Journal
eHST 33