Search Publications

Dense Molecular Clouds in the Crab Supernova Remnant
DOI: 10.3847/1538-4357/ac391a Bibcode: 2022ApJ...925...59W

Bentley, Rory O.; Fabian, A. C.; Combes, F. +7 more

Molecular emission was imaged with ALMA from numerous components near and within bright H2-emitting knots and absorbing dust globules in the Crab Nebula. These observations provide a critical test of how energetic photons and particles produced in a young supernova remnant interact with gas, cleanly differentiating between competing mod…

2022 The Astrophysical Journal
eHST 3
Dark Energy Camera photometry reveals extra-tidal stars around the Milky Way globular cluster NGC 6864 (M75)
DOI: 10.1093/mnras/stab3238 Bibcode: 2022MNRAS.509.3709P

Piatti, Andrés E.

Globular clusters are prone to lose stars while moving around the Milky Way. These stars escape the clusters and are distributed throughout extended envelopes or tidal tails. However, such extra-tidal structures are not observed in all globular clusters, and yet there are no structural or dynamical parameters that can predict their presence or abs…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 3
The Detection of Deuterated Water in the Large Magellanic Cloud with ALMA
DOI: 10.3847/1538-4357/ac6de1 Bibcode: 2022ApJ...933...64S

Oliveira, Joana M.; Chen, C. -H. Rosie; van Loon, Jacco Th. +10 more

We report the first detection of deuterated water (HDO) toward an extragalactic hot core. The HDO 211-212 line has been detected toward hot cores N 105-2 A and 2 B in the N 105 star-forming region in the low-metallicity Large Magellanic Cloud (LMC) dwarf galaxy with the Atacama Large Millimeter/submillimeter Array (ALMA). We …

2022 The Astrophysical Journal
Herschel 3
Simple interpretation of the seemingly complicated X-ray spectral variation of NGC 5548
DOI: 10.1093/mnras/stac1206 Bibcode: 2022MNRAS.513.5020M

Sugawara, Yasuharu; Ebisawa, Ken; Mizumoto, Misaki +1 more

NGC 5548 is a very well-studied Seyfert 1 galaxy in broad wavelengths. Previous multiwavelength observation campaigns have indicated that its multiple absorbers are highly variable and complex. A previous study applied a two-zone partial covering model with different covering fractions to explain the complex X-ray spectral variation and reported a…

2022 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 3
From Atmospheric Evolution to the Search of Species of Astrobiological Interest in the Solar System—Case Studies Using the Planetary Spectrum Generator
DOI: 10.3390/atmos13030461 Bibcode: 2022Atmos..13..461D

Machado, Pedro; Ribeiro, José; Dias, João A.

The study of minor chemical species in terrestrial planets' atmospheres can teach us about the chemistry, dynamics and evolution of the atmospheres through time. Phosphine or methane on terrestrial planets are potential biosignatures, such that their detection may signify the presence of life on a planet. Therefore, the search for these species in…

2022 Atmosphere
MEx 3
Earth through the looking glass: how frequently are we detected by other civilizations through photometric microlensing?
DOI: 10.1093/mnras/stac1855 Bibcode: 2022MNRAS.515.5927S

Robin, A. C.; Awiphan, S.; Kerins, E. +5 more

Microlensing is proving to be one of the best techniques to detect distant, low-mass planets around the most common stars in the Galaxy. In principle, Earth's microlensing signal could offer the chance for other technological civilizations to find the Earth across Galactic distances. We consider the photometric microlensing signal of Earth to othe…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 3
Detection of Extended Millimeter Emission in the Host Galaxy of 3C 273 and Its Implications for QSO Feedback via High Dynamic Range ALMA Imaging
DOI: 10.3847/1538-4357/ac616e Bibcode: 2022ApJ...930....3K

Saito, Toshiki; Toba, Yoshiki; Matsuoka, Yoshiki +2 more

We estimate the amount of negative feedback energy injected into the interstellar medium (ISM) of the host galaxy of 3C 273, a prototypical radio-loud quasar. We obtained 93, 233, and 343 GHz continuum images with the Atacama Large Millimeter/submillimeter Array (ALMA). After self-calibration and point-source subtraction, we reach an image dynamic…

2022 The Astrophysical Journal
eHST 3
Measurements of visual double stars with PISCO2 at the Nice 76-cm refractor in 2013-2014
DOI: 10.1002/asna.20224008 Bibcode: 2022AN....34324008G

Piccotti, Luca; Rivet, Jean-Pierre; Vakili, Farrokh +11 more

We present relative astrometric and photometric measurements of visual double stars made in 2013-2014 with PISCO2 installed at the 76-cm refractor of the Côte d'Azur Observatory in Nice (France). Our observation list contains orbital couples as well as double stars whose motion is still uncertain. Three different techniques were used for obtaining…

2022 Astronomische Nachrichten
Gaia 3
Hubble Space Telescope Imaging of Luminous Extragalactic Infrared Transients and Variables from the Spitzer Infrared Intensive Transients Survey
DOI: 10.3847/1538-4357/ac5832 Bibcode: 2022ApJ...928..158B

Gehrz, Robert D.; Bond, Howard E.; Bally, John +6 more

The SPitzer InfraRed Intensive Transients Survey (SPIRITS) searched for luminous infrared (IR) transients and variables in nearly 200 nearby galaxies from 2014 to 2019, using the warm Spitzer telescope at 3.6 and 4.5 µm. Among the SPIRITS variables are IR-bright objects that are undetected in ground-based optical surveys. We classify them as…

2022 The Astrophysical Journal
eHST 3
Refractory elements in the gas phase for comet 67P/Churyumov-Gerasimenko. Possible release of atomic Na, Si, and Fe from nanograins
DOI: 10.1051/0004-6361/202142209 Bibcode: 2022A&A...658A..87R

De Keyser, Johan; Gombosi, Tamas I.; Berthelier, Jean-Jacques +10 more

Context. Gas-phase sodium, silicon, potassium, and calcium were previously identified in mass spectra recorded in the coma of comet 67P/Churyumov-Gerasimenko, the target of the European Space Agency's Rosetta mission. The major release process for these atoms was identified as sputtering by the solar wind. More recently, remote observations of num…

2022 Astronomy and Astrophysics
Rosetta 3