L. Sabin
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View article: Discovery and classification of two new Galactic symbiotic stars in the IGAPS footprint
Discovery and classification of two new Galactic symbiotic stars in the IGAPS footprint Open
Symbiotic stars are considered astrophysical laboratories due to their complex physical and chemical properties. Despite theoretical predictions suggesting the existence of at least 1,200 such systems in the Galaxy, only 284 have been iden…
View article: A morphological catalogue of nova remnants
A morphological catalogue of nova remnants Open
This work presents the first optical imaging catalogue of resolved galactic nova remnants. It compiles images from proprietary observations carried out at the Nordic Optical Telescope and public archives using different telescopes and inst…
View article: A morphological catalogue of Nova Remnants
A morphological catalogue of Nova Remnants Open
This work presents the first optical imaging catalogue of resolved Galactic nova remnants. It compiles images from proprietary observations carried out at the Nordic Optical Telescope and public archives using different telescopes and inst…
View article: An attempt to determine the magnetic field configuration in the planetary nebula K 3-35 with ALMA
An attempt to determine the magnetic field configuration in the planetary nebula K 3-35 with ALMA Open
We examined dust polarization within the planetary nebula (PN) K 3-35 using the Atacama Large Millimeter/Submillimeter Array (ALMA). This investigation aimed to identify and trace the magnetic field within the PN, as it potentially plays a…
View article: High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The PANORAMA survey
High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The PANORAMA survey Open
As mass-losing asymptotic giant branch (AGB) stars evolve to planetary nebulae (PNe), the mass outflow geometries transform from nearly spherical to extreme aspherical. The physical mechanisms governing this transformation are widely belie…
View article: Shaping the nebula around the symbiotic system R Aquarii
Shaping the nebula around the symbiotic system R Aquarii Open
We present an analysis of high-dispersion spectroscopic observations of the symbiotic system R Aquarii (R Aqr) obtained with the Manchester Echelle Spectrograph at the 2.1-m telescope of the San Pedro Mártir Observatory (Mexico) in conjunc…
View article: Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3
Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3 Open
View article: 3D physical structure and angular expansion of the remnant of the recurrent nova T Pyx
3D physical structure and angular expansion of the remnant of the recurrent nova T Pyx Open
We present the analysis of archival Very Large Telescope (VLT) Multi-Unit Spectroscopic Explorer (MUSE) and multi-epoch Hubble Space Telescope (HST) Wide Field Planetary Camera 2 (WFPC2) and Wide Field Camera 3/Ultraviolet-Visible Imaging …
View article: Shaping the nebula around the symbiotic system R Aquarii
Shaping the nebula around the symbiotic system R Aquarii Open
We present an analysis of high-dispersion spectroscopic observations of the symbiotic system R Aquarii (R Aqr) obtained with the Manchester Echelle Spectrograph (MES) at the 2.1 m telescope of the San Pedro Mártir Observatory (Mexico). An …
View article: 3D physical structure and angular expansion of the remnant of the recurrent nova T Pyx
3D physical structure and angular expansion of the remnant of the recurrent nova T Pyx Open
We present the analysis of archival Very Large Telescope (VLT) MUSE and multi-epoch Hubble Space Telescope (HST) WFPC2 and WFC3/UVIS narrow-band observations of the remnant associated with the ejecta of the mid-nineteenth century outburst …
View article: TOI-663: A newly discovered multi-planet system with three transiting mini-Neptunes orbiting an early M star
TOI-663: A newly discovered multi-planet system with three transiting mini-Neptunes orbiting an early M star Open
We present the detection of three exoplanets orbiting the early M dwarf TOI-663 (TIC 54962195; V = 13.7 mag, J = 10.4 mag, R ★ = 0.512 ± 0.015 R ⊙ , M ★ = 0.514 ± 0.012 M ⊙ , d = 64 pc). TOI-663 b, c, and d, with respective radii of 2.27 ±…
View article: High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The PANORAMA survey
High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The PANORAMA survey Open
As AGB stars evolve to planetary nebulae (PNe), the geometry of the ejected mass transforms from nearly spherical to extremely aspherical. The mechanisms governing this transformation are plausibly linked to binarity and the associated pro…
View article: PB0146 Functional Characterization of a Human F9 Gene-Inserted Product in Hemophilia B Mice
PB0146 Functional Characterization of a Human F9 Gene-Inserted Product in Hemophilia B Mice Open
View article: TESS discovery of a super-Earth orbiting the M-dwarf star TOI-1680
TESS discovery of a super-Earth orbiting the M-dwarf star TOI-1680 Open
We report the discovery by the TESS mission of a super-Earth on a 4.8-days orbit around an inactive M4.5 dwarf (TOI-1680), validated by ground-based facilities. The host star is located 37.14 pc away, with a radius of 0.2100 ± 0.0064 R ⊙ ,…
View article: TOI-2084 b and TOI-4184 b: Two new sub-Neptunes around M dwarf stars
TOI-2084 b and TOI-4184 b: Two new sub-Neptunes around M dwarf stars Open
We present the discovery and validation of two TESS exoplanets orbiting nearby M dwarfs: TOI-2084 b, and TOI-4184b. We characterized the host stars by combining spectra from Shane /Kast and Magellan /FIRE, spectral energy distribution anal…
View article: TESS discovery of a super-Earth orbiting the M dwarf star TOI-1680
TESS discovery of a super-Earth orbiting the M dwarf star TOI-1680 Open
We report the discovery by the TESS mission of a super-Earth on a 4.8-d orbit around an inactive M4.5 dwarf (TOI-1680) validated by ground-based facilities. The host star is located 37.14 pc away, with a radius of 0.2100+/-0.0064 R_sun, ma…
View article: GJ 806 (TOI-4481): A bright nearby multi-planetary system with a transiting hot low-density super-Earth
GJ 806 (TOI-4481): A bright nearby multi-planetary system with a transiting hot low-density super-Earth Open
One of the main scientific goals of the TESS mission is the discovery of transiting small planets around the closest and brightest stars in the sky. Here, using data from the CARMENES, MAROON-X, and HIRES spectrographs together with TESS, …
View article: TOI-2084 b and TOI-4184 b: two new sub-Neptunes around M dwarf stars
TOI-2084 b and TOI-4184 b: two new sub-Neptunes around M dwarf stars Open
We present the discovery and validation of two TESS exoplanets orbiting nearby M dwarfs: TOI-2084b, and TOI-4184b. We characterized the host stars by combining spectra from Shane/Kast and Magellan/FIRE, SED (Spectral Energy Distribution) a…
View article: The origin of the planetary nebula M 1–16
The origin of the planetary nebula M 1–16 Open
We investigated the origin of the Planetary Nebula (PN) M 1–16 using narrow-band optical imaging, and high- and low-resolution optical spectra to perform a detailed morpho-kinematic and chemical studies. M 1–16 is revealed to be a multipol…
View article: The origin of the planetary nebula M 1-16. A morphokinematic and chemical analysis
The origin of the planetary nebula M 1-16. A morphokinematic and chemical analysis Open
We investigated the origin of the Planetary Nebula (PN) M 1-16 using narrow-band optical imaging, and high- and low-resolution optical spectra to perform a detailed morpho-kinematic and chemical studies. M 1-16 is revealed to be a multipol…
View article: Three-dimensional Orbit of AC Her Determined: Binary-induced Truncation Cannot Explain the Large Cavity in This Post-AGB Transition Disk
Three-dimensional Orbit of AC Her Determined: Binary-induced Truncation Cannot Explain the Large Cavity in This Post-AGB Transition Disk Open
Some evolved binaries, namely post–asymptotic giant branch (AGB) binaries, are surrounded by stable and massive circumbinary disks similar to protoplanetary disks found around young stars. Around 10% of these disks are transition disks: th…
View article: Peering into the central region of a nano-quasar: XMM-Newton and Chandra views of the CH Cyg Symbiotic System
Peering into the central region of a nano-quasar: XMM-Newton and Chandra views of the CH Cyg Symbiotic System Open
We present the analysis of archival XMM-Newton and Chandra observations of CH Cyg, one of the most studied symbiotic stars (SySts). The combination of the high-resolution XMM-Newton RGS and Chandra HETG X-ray spectra allowed us to obtain r…
View article: Three-dimensional orbit of AC Her determined: Binary-induced truncation cannot explain the large cavity in this post-AGB transition disk
Three-dimensional orbit of AC Her determined: Binary-induced truncation cannot explain the large cavity in this post-AGB transition disk Open
Some evolved binaries, namely post-asymptotic giant branch binaries, are surrounded by stable and massive circumbinary disks similar to protoplanetary disks found around young stars. Around 10% of these disks are transition disks: they hav…
View article: An XMM-Newton View of the Symbiotic Stars HM Sge, NQ Gem, and PU Vul
An XMM-Newton View of the Symbiotic Stars HM Sge, NQ Gem, and PU Vul Open
We present the analysis of archival XMM-Newton observations of the symbiotic stars HM Sge, NQ Gem, and PU Vul. The EPIC-pn spectra hint at the presence of emission lines, which are further confirmed in the first-order RGS spectra of the th…
View article: Surface magnetism in the pulsating RV Tauri star R Scuti
Surface magnetism in the pulsating RV Tauri star R Scuti Open
We present the surface magnetic field conditions of the brightest pulsating RV Tauri star, R Sct. Our investigation is based on the longest spectropolarimetric survey ever performed on this variable star. The analysis of high resolution sp…
View article: A super-Earth and a mini-Neptune near the 2:1 MMR straddling the radius valley around the nearby mid-M dwarf TOI-2096
A super-Earth and a mini-Neptune near the 2:1 MMR straddling the radius valley around the nearby mid-M dwarf TOI-2096 Open
Context. Several planetary formation models have been proposed to explain the observed abundance and variety of compositions of super-Earths and mini-Neptunes. In this context, multitransiting systems orbiting low-mass stars whose planets …
View article: GJ 806 (TOI-4481): A bright nearby multi-planetary system with a transiting hot, low-density super-Earth
GJ 806 (TOI-4481): A bright nearby multi-planetary system with a transiting hot, low-density super-Earth Open
One of the main scientific goals of the TESS mission is the discovery of transiting small planets around the closest and brightest stars in the sky. Here, using data from the CARMENES, MAROON-X, and HIRES spectrographs, together with TESS,…
View article: The messy death of a multiple star system and the resulting planetary nebula as observed by JWST
The messy death of a multiple star system and the resulting planetary nebula as observed by JWST Open
Planetary nebulae (PNe), the ejected envelopes of red giant stars, provide us with a history of the last, mass-losing phases of 90 percent of stars initially more massive than the Sun. Here, we analyse James Webb Space Telescope (JWST) Ear…
View article: Author Correction: The messy death of a multiple star system and the resulting planetary nebula as observed by JWST
Author Correction: The messy death of a multiple star system and the resulting planetary nebula as observed by JWST Open
View article: The messy death of a multiple star system and the resulting planetary nebula as observed by JWST
The messy death of a multiple star system and the resulting planetary nebula as observed by JWST Open