Search Publications

HST/WFC3 Hα Direct-imaging Detection of a Pointlike Source in the Disk Cavity of AB Aur
DOI: 10.3847/2041-8213/ac7fef Bibcode: 2022ApJ...934L..13Z

Zhou, Yifan; Kraus, Adam L.; Bae, Jaehan +8 more

Accreting protoplanets enable the direct characterization of planet formation. As part of a high-contrast imaging search for accreting planets with the Hubble Space Telescope (HST) Wide Field Camera 3, we present Hα images of AB Aurigae (AB Aur), a Herbig Ae/Be star harboring a transition disk. The data were collected in two epochs of direct-imagi…

2022 The Astrophysical Journal
eHST 38
A persistent ultraviolet outflow from an accreting neutron star binary transient
DOI: 10.1038/s41586-021-04324-2 Bibcode: 2022Natur.603...52C

Díaz Trigo, M.; Altamirano, D.; Knigge, C. +31 more

All disc-accreting astrophysical objects produce powerful disc winds. In compact binaries containing neutron stars or black holes, accretion often takes place during violent outbursts. The main disc wind signatures during these eruptions are blue-shifted X-ray absorption lines, which are preferentially seen in disc-dominated `soft states'1,2<…

2022 Nature
eHST 38
Observation of a Magnetic Switchback in the Solar Corona
DOI: 10.3847/2041-8213/ac8104 Bibcode: 2022ApJ...936L..25T

Telloni, Daniele; Zank, Gary P.; Adhikari, Laxman +58 more

Switchbacks are sudden, large radial deflections of the solar wind magnetic field, widely revealed in interplanetary space by the Parker Solar Probe. The switchbacks' formation mechanism and sources are still unresolved, although candidate mechanisms include Alfvénic turbulence, shear-driven Kelvin-Helmholtz instabilities, interchange reconnection…

2022 The Astrophysical Journal
SolarOrbiter 38
Stellar metallicity gradients of Local Group dwarf galaxies
DOI: 10.1051/0004-6361/202243508 Bibcode: 2022A&A...665A..92T

Jablonka, P.; Battaglia, G.; Taibi, S. +5 more


Aims: We explore correlations between the strength of metallicity gradients in Local Group dwarf galaxies and their stellar mass, star formation history timescales, and environment.
Methods: We performed a homogeneous analysis of literature spectroscopic data of red giant stars and determined radial metallicity profiles for 30 Local Grou…

2022 Astronomy and Astrophysics
Gaia 38
Red Spiral Galaxies at Cosmic Noon Unveiled in the First JWST Image
DOI: 10.3847/2041-8213/ac982b Bibcode: 2022ApJ...938L..24F

Inoue, Akio K.; Sugahara, Yuma; Fudamoto, Yoshinobu

In the first image of the James Webb Space Telescope (JWST) of SMACS J0723.3-7327, one of the most outstanding features is the emergence of a large number of red spiral galaxies, because such red spiral galaxies are only a few percent in the number fraction among nearby spiral galaxies. While these apparently red galaxies were already detected wit…

2022 The Astrophysical Journal
eHST JWST 38
TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf
DOI: 10.3847/1538-3881/ac7cea Bibcode: 2022AJ....164...96C

Latham, David W.; Tamura, Motohide; Stassun, Keivan G. +53 more

Exploring the properties of exoplanets near or inside the radius valley provides insight on the transition from the rocky super-Earths to the larger, hydrogen-rich atmosphere mini-Neptunes. Here, we report the discovery of TOI-1452b, a transiting super-Earth (R p = 1.67 ± 0.07 R ) in an 11.1 day temperate orbit (T eq

2022 The Astronomical Journal
Gaia 38
Opening the Era of Quasar-host Studies at High Redshift with JWST
DOI: 10.3847/2041-8213/ac9c02 Bibcode: 2022ApJ...939L..28D

Onoue, Masafusa; Silverman, John D.; Ding, Xuheng

We measure the host galaxy properties of five quasars with z ~ 1.6-3.5 selected from the Sloan Digital Sky Survey (SDSS) and AEGIS, which fall within the JWST/Hubble Space Telescope (HST) CEERS survey area. A point-spread function library is constructed based on stars in the full field of view of the data and used with the 2D image modeling tool g…

2022 The Astrophysical Journal
Gaia eHST JWST 38
Metallicities in M dwarfs: Investigating different determination techniques
DOI: 10.1051/0004-6361/202141920 Bibcode: 2022A&A...658A.194P

Amado, P. J.; Caballero, J. A.; Reiners, A. +17 more

Deriving metallicities for solar-like stars follows well-established methods, but for cooler stars such as M dwarfs, the determination is much more complicated due to forests of molecular lines that are present. Several methods have been developed in recent years to determine accurate stellar parameters for these cool stars (Teff ≲ 4000…

2022 Astronomy and Astrophysics
Gaia 38
Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey II: measurements in Fourier space with optimal weights
DOI: 10.1093/mnras/stac812 Bibcode: 2022MNRAS.514.3396M

Brownstein, Joel R.; Palanque-Delabrouille, Nathalie; Schneider, Donald P. +12 more

We present measurements of the local primordial non-Gaussianity parameter $f_{\mathrm{NL}}^\mathrm{local} $from the clustering of 343 708 quasars with redshifts 0.8 < z < 2.2 distributed over 4808 deg2 from the final data release (DR16) of the extended Baryon Acoustic Oscillation Spectroscopic Survey (eBOSS), the largest volume sp…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 38
The iron and oxygen content of LMC Classical Cepheids and its implications for the extragalactic distance scale and Hubble constant. Equivalent width analysis with Kurucz stellar atmosphere models
DOI: 10.1051/0004-6361/202142441 Bibcode: 2022A&A...658A..29R

Mucciarelli, Alessio; Riess, Adam; Yuan, Wenlong +6 more

Context. Classical Cepheids are primary distance indicators and a crucial stepping stone in determining the present-day value of the Hubble constant H0 to the precision and accuracy required to constrain apparent deviations from the ΛCDM Concordance Cosmological Model.
Aims: We measured the iron and oxygen abundances of a statistic…

2022 Astronomy and Astrophysics
Gaia 38