Search Publications

Luminosities and Masses of Single Galactic Post-asymptotic Giant Branch Stars with Distances from Gaia EDR3: The Revelation of an s-process Diversity
DOI: 10.3847/2041-8213/ac5686 Bibcode: 2022ApJ...927L..13K

Ventura, Paolo; Van Winckel, Hans; Hrivnak, Bruce J. +4 more

Post-asymptotic giant branch (AGB) stars are exquisite probes of AGB nucleosynthesis. However, the previous lack of accurate distances jeopardized comparison with theoretical AGB models. The Gaia Early Data Release 3 (Gaia EDR3) has now allowed for a breakthrough in this research landscape. In this study, we focus on a sample of single Galactic po…

2022 The Astrophysical Journal
Gaia 24
Complex Modulation of Rapidly Rotating Young M Dwarfs: Adding Pieces to the Puzzle
DOI: 10.3847/1538-3881/ac503c Bibcode: 2022AJ....163..144G

Jayaraman, Rahul; Kristiansen, Martti H.; Triaud, Amaury H. M. J. +37 more

New sets of young M dwarfs with complex, sharp-peaked, and strictly periodic photometric modulations have recently been discovered with Kepler/K2 (scallop shells) and TESS (complex rotators). All are part of star-forming associations, are distinct from other variable stars, and likely belong to a unified class. Suggested hypotheses include starspo…

2022 The Astronomical Journal
Gaia 24
Intrinsic Lyα Profiles of High-velocity G, K, and M Dwarfs
DOI: 10.3847/1538-4357/ac4711 Bibcode: 2022ApJ...926..129Y

Redfield, Seth; France, Kevin; Youngblood, Allison +5 more

Observations of H I Lyman α, the brightest UV emission line of late-type stars, are critical for understanding stellar chromospheres and transition regions, modeling photochemistry in exoplanet atmospheres, and measuring the abundances of neutral hydrogen and deuterium in the interstellar medium. Yet Lyα observations are notoriously challenging ow…

2022 The Astrophysical Journal
Gaia IRIS SOHO eHST 24
Modeling the kinematics of globular cluster systems
DOI: 10.1093/mnras/stac1651 Bibcode: 2022MNRAS.514.4736C

Chen, Yingtian; Gnedin, Oleg Y.

Globular clusters (GCs) are old massive star clusters that serve as 'fossils' of galaxy formation. The advent of Gaia observatory has enabled detailed kinematics studies of the Galactic GCs and revolutionized our understanding of the connections between GC properties and galaxy assembly. However, lack of kinematic measurements of extragalactic GCs…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 24
Found: a rapidly spinning white dwarf in LAMOST J024048.51+195226.9.
DOI: 10.1093/mnrasl/slab116 Bibcode: 2022MNRAS.509L..31P

Dhillon, V. S.; Breedt, E.; Marsh, T. R. +9 more

We present optical photometry of the cataclysmic variable LAMOST J024048.51+195226.9 taken with the high-speed, five-band CCD camera HiPERCAM on the 10.4 m Gran Telescopio Canarias (GTC). We detect pulsations originating from the spin of its white dwarf, finding a spin period of 24.9328(38)s. The pulse amplitude is of the order of 0.2% in the g-ba…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 24
Survey of Multiple Populations in Globular Clusters among Very-low-mass Stars
DOI: 10.3847/1538-4357/ac5046 Bibcode: 2022ApJ...927..207D

Milone, A. P.; Cordoni, G.; Marino, A. F. +14 more

Recent work has shown that near-infrared (NIR) Hubble Space Telescope (HST) photometry allows us to disentangle multiple populations (MPs) among M dwarfs of globular clusters (GCs) and to investigate this phenomenon in very-low-mass (VLM) stars. Here, we present the color-magnitude diagrams of nine GCs and the open cluster NGC 6791 in the F110W an…

2022 The Astrophysical Journal
eHST 24
Helium absorption in exoplanet atmospheres is connected to stellar coronal abundances
DOI: 10.1093/mnras/stac507 Bibcode: 2022MNRAS.512.1751P

Poppenhaeger, K.

Transit observations in the helium triplet around 10 830 Angstrom are a successful tool to study exoplanetary atmospheres and their mass loss. Forming those lines requires ionization and recombination of helium in the exoplanetary atmosphere. This ionization is caused by stellar photons at extreme ultraviolet (EUV) wavelengths; however, no current…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 24
The Close AGN Reference Survey (CARS). No obvious signature of AGN feedback on star formation, but subtle trends
DOI: 10.1051/0004-6361/202142011 Bibcode: 2022A&A...659A.125S

Gaspari, M.; Klessen, R. S.; Combes, F. +17 more

Context. Active galactic nuclei (AGN) are thought to be responsible for the suppression of star formation in massive ∼1010 M galaxies. While this process is a key feature in numerical simulations of galaxy formation, it has not been unambiguously confirmed in observational studies yet.
Aims: The characterization of the …

2022 Astronomy and Astrophysics
AKARI 24
Constraining the Nature of the 18 min Periodic Radio Transient GLEAM-X J162759.5-523504.3 via Multiwavelength Observations and Magneto-thermal Simulations
DOI: 10.3847/1538-4357/ac97ea Bibcode: 2022ApJ...940...72R

de Martino, D.; Rea, N.; Buckley, D. A. H. +14 more

We observed the periodic radio transient GLEAM-X J162759.5-523504.3 (GLEAM-X J1627) using the Chandra X-ray Observatory for about 30 ks on 2022 January 22-23, simultaneously with radio observations from the Murchison Widefield Array, MeerKAT, and the Australia Telescope Compact Array. Its radio emission and 18 min periodicity led the source to be …

2022 The Astrophysical Journal
Gaia 24
The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). II. The Spatially Resolved Recent Star Formation History of M33
DOI: 10.3847/1538-4357/ac7568 Bibcode: 2022ApJ...934...76L

Bell, Eric F.; Williams, Benjamin F.; Choi, Yumi +11 more

We measure the spatially resolved recent star formation history (SFH) of M33 using optical images taken with the Hubble Space Telescope as part of the Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER) survey. The area covered by the observations used in this analysis covers a de-projected area of ~38 kpc2 and …

2022 The Astrophysical Journal
eHST 24