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Uncovering the ultimate planet impostor. An eclipsing brown dwarf in a hierarchical triple with two evolved stars
DOI: 10.1051/0004-6361/202141158 Bibcode: 2021A&A...653A..40L

Montesinos, B.; Bouy, H.; Barrado, D. +14 more

Context. Exoplanet searches through space-based photometric time series have shown to be very efficient in recent years. However, follow-up efforts on the detected planet candidates have been demonstrated to be critical to uncover the true nature of the transiting objects.
Aims: In this paper we show a detailed analysis of one of those false …

2021 Astronomy and Astrophysics
Gaia 6
Extremely weak CO emission in IZw 18
DOI: 10.1051/0004-6361/202039033 Bibcode: 2021A&A...653L..10Z

Wang, Junzhi; Zhang, Zhi-Yu; Shi, Yong +1 more

Local metal-poor galaxies are ideal analogues of primordial galaxies with the interstellar medium (ISM) barely being enriched with metals. However, it is unclear whether carbon monoxide remains a good tracer and coolant of molecular gas at low metallicity. Based on the observation with the upgraded Northern Extended Millimeter Array, we report a m…

2021 Astronomy and Astrophysics
eHST 6
The Carina Nebula and Gum 31 Molecular Complex. III. The Distribution of the 1-3 GHz Radio Continuum across the Whole Nebula
DOI: 10.3847/1538-4357/abd7a3 Bibcode: 2021ApJ...909...93R

Garay, Guido; Breen, Shari L.; Rebolledo, David +2 more

We report the most detailed 1-3 GHz radio continuum emission map of the nearest region of massive-star formation, the Carina Nebula. As part of a large program with the Australia Telescope Compact Array, we have covered ∼12 deg2, achieving an angular resolution of ∼16″, representing the largest and most complete map of the radio continu…

2021 The Astrophysical Journal
Herschel 6
Re-Analysis of the Cassini RPWS/LP Data in Titan's Ionosphere: 1. Detection of Several Electron Populations
DOI: 10.1029/2020JA028412 Bibcode: 2021JGRA..12628412C

Wahlund, J. -E.; Edberg, N. J. T.; Hadid, L. Z. +5 more

Current models of Titan's ionosphere have difficulties in explaining the observed electron density and/or temperature. In order to get new insights, we re-analyzed the data taken in the ionosphere of Titan by the Cassini Langmuir probe (LP), part of the Radio and Plasma Wave Science (RPWS) instrument. This is the first of two papers that present t…

2021 Journal of Geophysical Research (Space Physics)
Cassini 6
Observation of bi-directional jets in a prominence
DOI: 10.1051/0004-6361/201935774 Bibcode: 2021A&A...651A..60H

Polito, V.; Hillier, A.

Quiescent prominences host a large range of flows, many driven by buoyancy, which lead to velocity shear. The presence of these shear flows could bend and stretch the magnetic field resulting in the formation of current sheets which can lead to magnetic reconnection. Though this has been hypothesised to occur in prominences, with some observations…

2021 Astronomy and Astrophysics
IRIS 6
Spectroscopic Monitoring of the Candidate Tidal Disruption Event in F01004-2237
DOI: 10.3847/1538-4357/abe049 Bibcode: 2021ApJ...909..159C

Jonker, Peter G.; Cannizzaro, Giacomo; Mata-Sánchez, D.

We present results of spectroscopic monitoring observations of the ultraluminous infrared galaxy F01004-2237. This galaxy was observed to undergo changes in its optical spectrum, detected by comparing a spectrum from 2015 with one from 2000. These changes were coincident with photometric brightening. The main changes detected in the optical spectr…

2021 The Astrophysical Journal
eHST 6
The Fundamental Plane of Massive Quiescent Galaxies at z ∼ 2
DOI: 10.3847/1538-4357/abce66 Bibcode: 2021ApJ...908..135S

Conselice, Christopher J.; Gallazzi, Anna; Zibetti, Stefano +11 more

We examine the Fundamental Plane (FP) and mass-to-light ratio (M/L) scaling relations using the largest sample of massive quiescent galaxies at 1.5 < z < 2.5 to date. The FP (re, σe, Ie) is established using 19 UVJ quiescent galaxies from COSMOS with Hubble Space Telescope HF160W rest-frame optical…

2021 The Astrophysical Journal
eHST 6
Are we observing an NSC in course of formation in the NGC 4654 galaxy?
DOI: 10.1093/mnras/stab458 Bibcode: 2021MNRAS.503..594S

Mastrobuono-Battisti, A.; Georgiev, I. Y.; Capuzzo-Dolcetta, R. +2 more

We use direct N-body simulations to explore some possible scenarios for the future evolution of two massive clusters observed towards the centre of NGC 4654, a spiral galaxy with mass similar to that of the Milky Way. Using archival HST data, we obtain the photometric masses of the two clusters, M = 3 × 105 M and M = 1.7 × 1…

2021 Monthly Notices of the Royal Astronomical Society
eHST 6
Low-frequency Waves due to Newborn Interstellar Pickup He+ Observed by the Ulysses Spacecraft
DOI: 10.3847/1538-4357/ac2eb3 Bibcode: 2021ApJ...923..185M

Isenberg, Philip A.; Schwadron, Nathan A.; Murphy, Neil +8 more

We have surveyed magnetic field data from the Ulysses spacecraft and found examples of magnetic waves with the expected characteristics that point to excitation by newborn pickup He+. With interstellar neutrals as the likely source for the pickup ions, we have modeled the ion production rates and used them to produce wave excitation rat…

2021 The Astrophysical Journal
Ulysses 6
Seeking Echoes of Circumstellar Disks in Kepler Light Curves
DOI: 10.3847/1538-3881/ac05be Bibcode: 2021AJ....162...98B

Kenyon, Scott J.; Bromley, Benjamin C.; Leonard, Austin +3 more

Light echoes of flares on active stars offer the opportunity for direct detection of circumstellar dust. We revisit the problem of identifying faint echoes in postflare light curves, focusing on debris disks from ongoing planet formation. Starting with simulations, we develop an algorithm for estimating the radial extent and total mass from disk e…

2021 The Astronomical Journal
Gaia 6