Search Publications

Volatile exposures on the 67P/Churyumov-Gerasimenko nucleus
DOI: 10.1051/0004-6361/202245614 Bibcode: 2023A&A...672A.136F

Fulle, M.; Fornasier, S.; Ciarniello, M. +2 more


Aims: We present the most extensive catalog of exposures of volatiles on the 67P/Churyumov-Gerasimenko nucleus generated from observations acquired with the Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) on board the Rosetta mission. We investigate the volatile exposure distribution across the nucleus, their size distribu…

2023 Astronomy and Astrophysics
Rosetta 13
The MUSCLES Extension for Atmospheric Transmission Spectroscopy: UV and X-Ray Host-star Observations for JWST ERS & GTO Targets
DOI: 10.3847/1538-3881/acdb70 Bibcode: 2023AJ....166...35B

Brown, Alexander; France, Kevin; Youngblood, Allison +8 more

X-ray through infrared spectral energy distributions (SEDs) are essential for understanding a star's effect on exoplanet atmospheric composition and evolution. We present a catalog of panchromatic SEDs, hosted on the Barbara A. Mikulski Archive for Space Telescopes, for 11 exoplanet-hosting stars that have guaranteed JWST observation time as part …

2023 The Astronomical Journal
Gaia XMM-Newton eHST 13
The edge-on protoplanetary disk HH 48 NE. I. Modeling the geometry and stellar parameters
DOI: 10.1051/0004-6361/202346052 Bibcode: 2023A&A...677A..17S

Rocha, W. R. M.; Dartois, E.; McClure, M. K. +11 more

Context. Observations of edge-on disks are an important tool for constraining general protoplanetary disk properties that cannot be determined in any other way. However, most radiative transfer models cannot simultaneously reproduce the spectral energy distributions (SEDs) and resolved scattered light and submillimeter observations of these system…

2023 Astronomy and Astrophysics
eHST JWST 13
The Eclipsing Binaries from the LAMOST Medium-resolution Survey. III. A High-precision Empirical Stellar Mass Library
DOI: 10.3847/1538-3881/aca288 Bibcode: 2023AJ....165...30X

Li, Jiadong; Xiong, Jianping; Liu, Chao +6 more

High-precision stellar masses and radii measured directly from binaries can effectively calibrate stellar models. However, such a database containing full spectral types and a large range of metallicity is still not fully established. A continuous effort of data collection and analysis is requested to complete the database. In this work, we provid…

2023 The Astronomical Journal
Gaia 13
Late-time HST UV and optical observations of AT 2018cow: extracting a cow from its background
DOI: 10.1093/mnras/stad2531 Bibcode: 2023MNRAS.525.4042I

Jonker, Peter G.; Perley, Daniel A.; Mummery, Andrew +4 more

The bright, blue, rapidly evolving AT 2018cow is a well-studied peculiar extragalactic transient. Despite an abundance of multiwavelength data, there still is no consensus on the nature of the event. We present our analysis of three epochs of Hubble Space Telescope (HST) observations spanning the period from 713 to 1474 d post-burst, paying partic…

2023 Monthly Notices of the Royal Astronomical Society
eHST 13
IXPE and XMM-Newton Observations of the Soft Gamma Repeater SGR 1806-20
DOI: 10.3847/1538-4357/aced05 Bibcode: 2023ApJ...954...88T

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +96 more

Recent observations with the Imaging X-ray Polarimetry Explorer (IXPE) of two anomalous X-ray pulsars provided evidence that X-ray emission from magnetar sources is strongly polarized. Here we report on the joint IXPE and XMM-Newton observations of the soft γ-repeater SGR 1806-20. The spectral and timing properties of SGR 1806-20 derived from XMM-…

2023 The Astrophysical Journal
XMM-Newton 13
Absence of nuclear polycyclic aromatic hydrocarbon emission from a compact starburst: The case of the type-2 quasar Mrk 477
DOI: 10.1051/0004-6361/202245409 Bibcode: 2023A&A...669L...5R

Rigopoulou, D.; Tadhunter, C. N.; Acosta-Pulido, J. A. +11 more

Mrk 477 is the closest type-2 quasar, at a distance of 163 Mpc. This makes it an ideal laboratory for studying the interplay between nuclear activity and star formation with a great level of detail and signal-to-noise. In this Letter we present new mid-infrared (mid-IR) imaging and spectroscopic data with an angular resolution of 0.4″ (∼300 pc) ob…

2023 Astronomy and Astrophysics
eHST 13
The Large Array Survey Telescope-Science Goals
DOI: 10.1088/1538-3873/aceb30 Bibcode: 2023PASP..135h5002B

Gal-Yam, A.; Rybicki, K.; Sadeh, I. +21 more

The Large Array Survey Telescope (LAST) is designed to survey the variable and transient sky at high temporal cadence. The array is comprised of 48 F/2.2 telescopes of 27.9 cm aperture, coupled to full-frame backside-illuminated cooled CMOS detectors with 3.76 µm pixels, resulting in a pixel scale of 1.″25. A single telescope with a field of…

2023 Publications of the Astronomical Society of the Pacific
Gaia 13
Volatiles in the H2O and CO2 ices of comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stad3005 Bibcode: 2023MNRAS.526.4209R

De Keyser, Johan; Gombosi, Tamas I.; Berthelier, Jean-Jacques +11 more

European Space Agency's Rosetta spacecraft at comet 67P/Churyumov-Gerasimenko (67P) was the first mission that accompanied a comet over a substantial fraction of its orbit. On board was the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis mass spectrometer suite to measure the local densities of the volatile species sublimating from the i…

2023 Monthly Notices of the Royal Astronomical Society
Rosetta 13
Measurement of the Angular Momenta of Pre-main-sequence Stars: Early Evolution of Slow and Fast Rotators and Empirical Constraints on Spin-down Torque Mechanisms
DOI: 10.3847/1538-3881/acc2bd Bibcode: 2023AJ....165..182K

Stassun, Keivan G.; Kounkel, Marina; Hillenbrand, Lynne A. +3 more

We use TESS full-frame imaging data to investigate the angular momentum evolution of young stars in the Orion Complex. We confirm recent findings that stars with rotation periods faster than 2 days are overwhelmingly binaries, with typical separations of tens of au; such binaries quickly clear their disks, leading to a tendency for rapid rotators …

2023 The Astronomical Journal
Gaia 13