Search Publications

Physical properties of the trans-Neptunian object (38628) Huya from a multi-chord stellar occultation
DOI: 10.1051/0004-6361/202141546 Bibcode: 2022A&A...664A.130S

Ofek, E.; Marques Oliveira, J.; Sicardy, B. +85 more

Context. As part of our international program aimed at obtaining accurate physical properties of trans-Neptunian objects (TNOs), we predicted a stellar occultation by the TNO (38628) Huya of the star Gaia DR2 4352760586390566400 (mG = 11.5 mag) on March 18, 2019. After an extensive observational campaign geared at obtaining the astromet…

2022 Astronomy and Astrophysics
Gaia 12
Detectability of Rotational Modulation in Kepler Sun-like Stars as a Function of Age
DOI: 10.3847/1538-4357/ac8d58 Bibcode: 2022ApJ...937...94M

Masuda, Kento

We examine how the fraction f of stars for which rotational modulation has been detected in Kepler light curves depends on the stellar mass M and age t . Our sample consists of ≈850 FGK stars hosting transiting planet candidates detected from the prime Kepler mission. For these stars, atmospheric parameters have been deriv…

2022 The Astrophysical Journal
Gaia 12
Phobos and Deimos surface composition: search for spectroscopic analogues
DOI: 10.1093/mnras/stac2226 Bibcode: 2022MNRAS.516..465P

Barucci, M. A.; Fornasier, S.; Matsuoka, M. +6 more

Phobos and Deimos, the two satellites of Mars, were largely studied in the past using ground-based telescope and spacecraft data, although most of the data were obtained by opportunity observations performed by Mars dedicated orbiters. Despite the data available so far, the main composition of the two moons is not yet fully understood. The possibl…

2022 Monthly Notices of the Royal Astronomical Society
MEx 12
Measuring the Orbits of the Arches and Quintuplet Clusters Using HST and Gaia: Exploring Scenarios for Star Formation near the Galactic Center
DOI: 10.3847/1538-4357/ac8bd6 Bibcode: 2022ApJ...939...68H

Lu, Jessica R.; Anderson, Jay; Morris, Mark R. +4 more

We present new absolute proper-motion measurements for the Arches and Quintuplet clusters, two young massive star clusters near the Galactic center. Using multiepoch HST observations, we construct proper-motion catalogs for the Arches (~35,000 stars) and Quintuplet (~40,000 stars) fields in ICRF coordinates established using stars in common with t…

2022 The Astrophysical Journal
Gaia eHST 12
Extreme-Ultraviolet Wave and Accompanying Loop Oscillations
DOI: 10.1007/s11207-022-02082-6 Bibcode: 2022SoPh..297..153D

Awasthi, Arun Kumar; Schmieder, Brigitte; Joshi, Reetika +2 more

We present the observations of an extreme-ultraviolet (EUV) wave, which originated from the active region (AR) NOAA 12887 on 28 October 2021, and its impact on neighboring loops. The event was observed by the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO) satellite at various wavebands and by the Solar TErrestrial…

2022 Solar Physics
SOHO 12
Protracted Hydrogeological Activity in Arabia Terra, Mars: Evidence From the Structure and Mineralogy of the Layered Deposits of Becquerel Crater
DOI: 10.1029/2022JE007320 Bibcode: 2022JGRE..12707320S

Rossi, A. P.; Pondrelli, M.; Schmidt, G. +3 more

The formation of layered mounds on Mars remains a major topic of debate, with the relationship between their deposition and chemical alteration a major aspect still to be constrained. The association these deposits have with hydrated minerals indicates aqueous processes were active in their past, however the extent and duration of this aqueous per…

2022 Journal of Geophysical Research (Planets)
MEx 12
Stellar Chromospheric Activity Database of Solar-like Stars Based on the LAMOST Low-Resolution Spectroscopic Survey
DOI: 10.3847/1538-4365/ac9406 Bibcode: 2022ApJS..263...12Z

Zhang, Jun; Zhang, Haotong; Luo, Ali +3 more

A stellar chromospheric activity database of solar-like stars is constructed based on the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Low-Resolution Spectroscopic Survey. The database contains spectral bandpass fluxes and indexes of Ca II H and K lines derived from 1,330,654 high-quality LRS spectra of solar-like stars. We m…

2022 The Astrophysical Journal Supplement Series
Gaia 12
COLDz: Probing Cosmic Star Formation With Radio Free-Free Emission
DOI: 10.3847/1538-4357/ac34f5 Bibcode: 2022ApJ...924...76A

Dickinson, Mark; Smail, Ian; Daddi, Emanuele +17 more

Radio free-free emission is considered to be one of the most reliable tracers of star formation in galaxies. However, as it constitutes the faintest part of the radio spectrum-being roughly an order of magnitude less luminous than radio synchrotron emission at the GHz frequencies typically targeted in radio surveys-the usage of free-free emission …

2022 The Astrophysical Journal
eHST 12
Panchromatic HST/WFC3 Imaging Studies of Young, Rapidly Evolving Planetary Nebulae. I. NGC 6302
DOI: 10.3847/1538-4357/ac51cd Bibcode: 2022ApJ...927..100K

Montez, Rodolfo; Frank, Adam; Balick, Bruce +4 more

We present the results of a comprehensive, near-UV-to-near-IR Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) imaging study of the young planetary nebula (PN) NGC 6302, the archetype of the class of extreme bilobed, pinched-waist PNe that are rich in dust and molecular gas. The new WFC3 emission-line image suite clearly defines the dusty t…

2022 The Astrophysical Journal
Gaia eHST 12
A GALAH view of the chemical homogeneity and ages of stellar strings identified in Gaia
DOI: 10.1093/mnras/stac236 Bibcode: 2022MNRAS.511.2829M

Hawkins, Keith; Maas, Zachary G.; Manea, Catherine

The advent of Gaia has led to the discovery of nearly 300 elongated stellar associations (called 'strings') spanning hundreds of parsecs in length and mere tens of parsecs in width. These newfound populations present an excellent laboratory for studying the assembly process of the Milky Way thin disc. In this work, we use data from GALAH DR3 to in…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 12