Search Publications

Constraints on the Spindown of Fully Convective M Dwarfs Using Wide Field Binaries
DOI: 10.3847/1538-4357/ac7da8 Bibcode: 2022ApJ...936..109P

Winters, Jennifer G.; Irwin, Jonathan M.; Charbonneau, David +1 more

M dwarfs remain active over longer timescales than their Sunlike counterparts, with potentially devastating implications for the atmospheres of their planets. However, the age at which fully convective M dwarfs transition from active and rapidly rotating to quiescent and slowly rotating is poorly understood, as these stars remain rapidly rotating …

2022 The Astrophysical Journal
Gaia 30
The Magellanic Edges Survey - II. Formation of the LMC's northern arm
DOI: 10.1093/mnras/stab3350 Bibcode: 2022MNRAS.510..445C

Da Costa, G. S.; Belokurov, V.; Koposov, S. E. +3 more

The highly-substructured outskirts of the Magellanic Clouds provide ideal locations for studying the complex interaction history between both Clouds and the Milky Way (MW). In this paper, we investigate the origin of a >20° long arm-like feature in the northern outskirts of the Large Magellanic Cloud (LMC) using data from the Magellanic Edges S…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 30
GOALS-JWST: Resolving the Circumnuclear Gas Dynamics in NGC 7469 in the Mid-infrared
DOI: 10.3847/2041-8213/ac961c Bibcode: 2022ApJ...940L...5U

Inami, Hanae; Böker, Torsten; Law, David R. +35 more

The nearby, luminous infrared galaxy NGC 7469 hosts a Seyfert nucleus with a circumnuclear star-forming ring and is thus the ideal local laboratory for investigating the starburst-AGN (active galactic nucleus) connection in detail. We present integral-field observations of the central 1.3 kpc region in NGC 7469 obtained with the JWST Mid-InfraRed …

2022 The Astrophysical Journal
JWST 30
Gemini-LIGHTS: Herbig Ae/Be and Massive T Tauri Protoplanetary Disks Imaged with Gemini Planet Imager
DOI: 10.3847/1538-3881/ac7be4 Bibcode: 2022AJ....164..109R

Monnier, John D.; Kraus, Stefan; Oppenheimer, Rebecca +20 more

We present the complete sample of protoplanetary disks from the Gemini- Large Imaging with the Gemini Planet Imager Herbig/T Tauri Survey, which observed bright Herbig Ae/Be stars and T Tauri stars in near-infrared polarized light to search for signatures of disk evolution and ongoing planet formation. The 44 targets were chosen based on their nea…

2022 The Astronomical Journal
Gaia 30
Flux rope and dynamics of the heliospheric current sheet. Study of the Parker Solar Probe and Solar Orbiter conjunction of June 2020
DOI: 10.1051/0004-6361/202142381 Bibcode: 2022A&A...659A.110R

Fedorov, A.; Parenti, S.; Lavraud, B. +19 more

Context. Solar Orbiter and Parker Solar Probe jointly observed the solar wind for the first time in June 2020, capturing data from very different solar wind streams: calm, Alfvénic wind and also highly dynamic large-scale structures. Context. Our aim is to understand the origin and characteristics of the highly dynamic solar wind observed by the t…

2022 Astronomy and Astrophysics
SolarOrbiter 30
Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone
DOI: 10.1051/0004-6361/202243164 Bibcode: 2022A&A...662A..16B

Gizon, Laurent; Cameron, Robert H.; Bekki, Yuto

Context. Several types of global-scale inertial modes of oscillation have been observed on the Sun. These include the equatorial Rossby modes, critical-latitude modes, and high-latitude modes. However, the columnar convective modes (predicted by simulations and also known as banana cells or thermal Rossby waves) remain elusive.
Aims: We aim t…

2022 Astronomy and Astrophysics
SOHO 30
Star-spots and magnetism: testing the activity paradigm in the Pleiades and M67
DOI: 10.1093/mnras/stac2706 Bibcode: 2022MNRAS.517.2165C

Pinsonneault, Marc H.; Cao, Lyra

We measure star-spot filling fractions for 240 stars in the Pleiades and M67 open star clusters using APOGEE high-resolution H-band spectra. For this work, we developed a modified spectroscopic pipeline which solves for star-spot filling fraction and star-spot temperature contrast. We exclude binary stars, finding that the large majority of binari…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 30
Milky Way mass with K giants and BHB stars using LAMOST, SDSS/SEGUE, and Gaia: 3D spherical Jeans equation and tracer mass estimator
DOI: 10.1093/mnras/stac2036 Bibcode: 2022MNRAS.516..731B

Bird, Sarah A.; Zhao, Gang; Tian, Hai-Jun +8 more

We measure the enclosed Milky Way mass profile to Galactocentric distances of ~70 and ~50 kpc using the smooth, diffuse stellar halo samples of Bird et al. The samples are Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) and Sloan Digital Sky Survey/Sloan Extension for Galactic Understanding and Exploration (SDSS/SEGUE) K giants …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 30
Solar coronal heating from small-scale magnetic braids
DOI: 10.1051/0004-6361/202244170 Bibcode: 2022A&A...667A.166C

Barczynski, K.; Peter, H.; Chitta, L. P. +19 more

Relaxation of braided coronal magnetic fields through reconnection is thought to be a source of energy to heat plasma in active region coronal loops. However, observations of active region coronal heating associated with an untangling of magnetic braids remain sparse. One reason for this paucity could be the lack of coronal observations with a suf…

2022 Astronomy and Astrophysics
Hinode SolarOrbiter 30
Detecting low-mass haloes with strong gravitational lensing I: the effect of data quality and lensing configuration
DOI: 10.1093/mnras/stab3537 Bibcode: 2022MNRAS.510.2480D

White, Simon D. M.; Fassnacht, Christopher D.; Rizzo, Francesca +5 more

This paper aims to quantify how the lowest halo mass that can be detected with galaxy-galaxy strong gravitational lensing depends on the quality of the observations and the characteristics of the observed lens systems. Using simulated data, we measure the lowest detectable NFW mass at each location of the lens plane, in the form of detailed sensit…

2022 Monthly Notices of the Royal Astronomical Society
eHST 30