Search Publications

Evidence of ram-pressure stripping of WLM, a dwarf galaxy far away from any large host galaxy
DOI: 10.1051/0004-6361/202243307 Bibcode: 2022A&A...660L..11Y

Józsa, Gyula I. G.; McConnachie, Alan W.; Hammer, Francois +5 more

Dwarf galaxies are affected by all the evolutionary processes normally at work in galaxies of any mass. As fainter and less massive galaxies, however, dwarf galaxies are particularly susceptible to environmental mechanisms that can more easily perturb these systems. Importantly, the presence of nearby large galaxies is expected to have a profound …

2022 Astronomy and Astrophysics
Gaia 16
Thermal and Nonthermal Emission in the Optical-UV Spectrum of PSR B0950+08
DOI: 10.3847/1538-4357/ac3a6f Bibcode: 2022ApJ...924..128A

Pavlov, George G.; Kargaltsev, Oleg; Abramkin, Vadim +1 more

Based on recent Hubble Space Telescope (HST) observations in the far-UV and ground-based observations in optical bands, Pavlov and colleagues have revealed a thermal component in the spectrum of the old pulsar B0950+08 (spin-down age 17.5 Myr) and estimated a neutron star (NS) surface temperature of (1-3) × 105 K. Our new HST observatio…

2022 The Astrophysical Journal
Gaia eHST 16
Understanding Accretion Variability through TESS Observations of Taurus
DOI: 10.3847/1538-4357/ac7e51 Bibcode: 2022ApJ...935...54R

Rodriguez, Joseph E.; Espaillat, Catherine C.; Robinson, Connor E.

Interpreting the short-timescale variability of the accreting, young, low-mass stars known as Classical T Tauri stars remains an open task. Month-long, continuous light curves from the Transiting Exoplanet Survey Satellite (TESS) have become available for hundreds of T Tauri stars. With this vast data set, identifying connections between the varia…

2022 The Astrophysical Journal
Gaia eHST 16
Beyond the Local Volume. I. Surface Densities of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
DOI: 10.3847/1538-4357/ac35ea Bibcode: 2022ApJ...924..114A

Holwerda, Benne; Burgasser, Adam J.; Ryan, Russell E. +6 more

Ultracool dwarf stars and brown dwarfs provide a unique probe of large-scale Galactic structure and evolution; however, until recently spectroscopic samples of sufficient size, depth, and fidelity have been unavailable. Here, we present the identification of 164 M7-T9 ultracool dwarfs in 0.6 deg2 of deep, low-resolution, near-infrared s…

2022 The Astrophysical Journal
Gaia eHST 16
The VVV survey: Long-period variable stars. I. Photometric catalog of ten VVV/OGLE tiles
DOI: 10.1051/0004-6361/202141805 Bibcode: 2022A&A...660A..35N

Minniti, D.; Zoccali, M.; Rojas-Arriagada, A. +7 more

Context. Long-period variable stars (LPVs) are pulsating red giants, primarily in the asymptotic giant branch phase, and they include both Miras and semi-regular variables (SRVs). Their period-age and period-luminosity relations enable us to trace different stellar populations, as they are intrinsically very bright and cover a wide range in distan…

2022 Astronomy and Astrophysics
Gaia 16
Callisto's Atmosphere: First Evidence for H2 and Constraints on H2O
DOI: 10.1029/2022JE007294 Bibcode: 2022JGRE..12707294C

Alday, Juan; Johnson, Robert E.; Roth, Lorenz +8 more

We explore the parameter space for the contribution to Callisto's H corona observed by the Hubble Space Telescope from sublimated H2O and radiolytically produced H2 using the Direct Simulation Monte Carlo method. The spatial morphology of this corona produced via photoelectron and magnetospheric electron-impact-induced dissoc…

2022 Journal of Geophysical Research (Planets)
eHST 16
The white dwarf binary pathways survey - VII. Evidence for a bi-modal distribution of post-mass transfer systems?
DOI: 10.1093/mnras/stac673 Bibcode: 2022MNRAS.512.2625L

Gänsicke, B. T.; Parsons, S. G.; Hernandez, M. S. +5 more

Binary systems consisting of a white dwarf (WD) and a main-sequence companion with orbital periods up to ≈100 d are often thought to be formed through common envelope evolution which is still poorly understood. To provide new observational constraints on the physical processes involved in the formation of these objects, we are conducting a large-s…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 16
Apsidal motion in massive eccentric binaries: The case of CPD-41° 7742, and HD 152218 revisited
DOI: 10.1051/0004-6361/202243707 Bibcode: 2022A&A...664A..98R

Gosset, E.; Sterken, C.; Nazé, Y. +2 more

Context. This paper is part of a study of the apsidal motion in close eccentric massive binary systems, which aims to constrain the internal structure of the stars. We focus on the binary CPD-41° 7742 and briefly revisit the case of HD 152218.
Aims: Independent studies of CPD-41° 7742 in the past showed large discrepancies in the longitude of…

2022 Astronomy and Astrophysics
Gaia 16
CLASSY V: The Impact of Aperture Effects on the Inferred Nebular Properties of Local Star-forming Galaxies
DOI: 10.3847/1538-4357/ac7854 Bibcode: 2022ApJ...935...74A

Martin, Crystal L.; Brinchmann, Jarle; Charlot, Stéphane +23 more

Strong nebular emission lines are an important diagnostic tool for tracing the evolution of star-forming galaxies across cosmic time. However, different observational setups can affect these lines, and the derivation of the physical nebular properties. We analyze 12 local star-forming galaxies from the COS Legacy Spectroscopy SurveY (CLASSY) to as…

2022 The Astrophysical Journal
eHST 16
SOFIA Observations of Far-IR Fine-structure Lines in Galaxies to Measure Metallicity
DOI: 10.3847/1538-4357/ac37b7 Bibcode: 2022ApJ...926...55S

Spinoglio, Luigi; Fernández-Ontiveros, Juan Antonio; Malkan, Matthew A. +8 more

We present new and archival SOFIA FIFI-LS far-IR spectroscopic observations of the [O III] 52 µm and/or the [N III] 57 µm lines of 25 local galaxies. Including 31 other galaxies from Herschel-PACS, we discuss a local sample of 47 galaxies, including the H II galaxies, luminous IR galaxies, low-metallicity dwarfs, and Seyfert nuclei. An…

2022 The Astrophysical Journal
Herschel ISO 16