Search Publications

The role of highly vibrationally excited H2 initiating the nitrogen chemistry. Quantum study and 3σ detection of NH emission in the Orion Bar PDR
DOI: 10.1051/0004-6361/202243884 Bibcode: 2022A&A...664A.190G

Goicoechea, Javier R.; Roncero, Octavio

The formation of hydrides by gas-phase reactions between H2 and a heavy element atom is a very selective process. Reactions with ground-state neutral carbon, oxygen, nitrogen, and sulfur atoms are very endoergic and have high energy barriers because the H2 molecule has to be fragmented before a hydride bond is formed. In cold…

2022 Astronomy and Astrophysics
Herschel 12
Is there a sub-parsec-scale jet base in the nearby dwarf galaxy NGC 4395?
DOI: 10.1093/mnras/stac1753 Bibcode: 2022MNRAS.514.6215Y

Ho, Luis C.; Paragi, Zsolt; Nyland, Kristina +6 more

NGC 4395 is a dwarf galaxy at a distance of about 4.3 Mpc (scale: ~0.021 pc mas-1). It hosts an intermediate-mass black hole (IMBH) with a mass between ~104 and ~105 solar masses. The early radio observations of NGC 4395 with the very long baseline interferometry (VLBI) network, High Sensitivity Array (HSA), at 1.4…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 12
Measuring chemical abundances in AGN from infrared nebular lines: HII-CHI-MISTRY-IR for AGN
DOI: 10.1051/0004-6361/202243602 Bibcode: 2022A&A...666A.115P

Pérez-Díaz, Borja; Pérez-Montero, Enrique; Fernández-Ontiveros, Juan A. +1 more

Context. Future and ongoing infrared and radio observatories such as JWST, METIS, and ALMA will increase the amount of rest-frame IR spectroscopic data for galaxies by several orders of magnitude. While studies of the chemical composition of the interstellar medium (ISM) based on optical observations have been widely spread over decades for star-f…

2022 Astronomy and Astrophysics
Herschel ISO 12
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