Search Publications

HATS-74Ab, HATS-75b, HATS-76b, and HATS-77b: Four Transiting Giant Planets Around K and M Dwarfs
DOI: 10.3847/1538-3881/ac4a77 Bibcode: 2022AJ....163..125J

Hobson, M.; Jordán, Andrés; Palle, E. +35 more

The relative rarity of giant planets around low-mass stars compared with solar-type stars is a key prediction from the core-accretion planet formation theory. In this paper we report on the discovery of four gas giant planets that transit low-mass late K and early M dwarfs. The planets HATS-74Ab (TOI 737b), HATS-75b (TOI 552b), HATS-76b (TOI 555b)…

2022 The Astronomical Journal
Gaia 35
The Rate, Amplitude, and Duration of Outbursts from Class 0 Protostars in Orion
DOI: 10.3847/2041-8213/ac46ae Bibcode: 2022ApJ...924L..23Z

Manoj, P.; Narang, Mayank; Pokhrel, Riwaj +18 more

At least half of a protostar's mass is accreted in the Class 0 phase, when the central protostar is deeply embedded in a dense, infalling envelope. We present the first systematic search for outbursts from Class 0 protostars in the Orion clouds. Using photometry from Spitzer/IRAC spanning 2004 to 2017, we detect three outbursts from Class 0 protos…

2022 The Astrophysical Journal
Herschel 35
COCONUT, a Novel Fast-converging MHD Model for Solar Corona Simulations: I. Benchmarking and Optimization of Polytropic Solutions
DOI: 10.3847/1538-4357/ac7237 Bibcode: 2022ApJ...936...19P

Poedts, Stefaan; Zhang, Fan; Perri, Barbara +5 more

We present a novel global 3D coronal MHD model called COCONUT, polytropic in its first stage and based on a time-implicit backward Euler scheme. Our model boosts run-time performance in comparison with contemporary MHD-solvers based on explicit schemes, which is particularly important when later employed in an operational setting for space-weather…

2022 The Astrophysical Journal
SOHO 35
Detection of a 100,000 M black hole in M31's Most Massive Globular Cluster: A Tidally Stripped Nucleus
DOI: 10.3847/1538-4357/ac339f Bibcode: 2022ApJ...924...48P

Pechetti, Renuka; Caldwell, Nelson; Kamann, Sebastian +6 more

We investigate the presence of a central black hole (BH) in B023-G078, M31's most massive globular cluster. We present high-resolution, adaptive-optics assisted, integral-field spectroscopic kinematics from Gemini/NIFS that show a strong rotation (~20 km s-1) and a velocity dispersion rise toward the center (37 km s-1). We co…

2022 The Astrophysical Journal
eHST 35
Variable star classification across the Galactic bulge and disc with the VISTA Variables in the Vía Láctea survey
DOI: 10.1093/mnras/stab3116 Bibcode: 2022MNRAS.509.2566M

Smith, Leigh C.; Belokurov, Vasily; Minniti, Dante +3 more

We present VIVACE, the VIrac VAriable Classification Ensemble, a catalogue of variable stars extracted from an automated classification pipeline for the Vista Variables in the Vía Láctea (VVV) infrared survey of the Galactic bar/bulge and southern disc. Our procedure utilizes a two-stage hierarchical classifier to first isolate likely variable sou…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 35
Blue Rest-frame UV-optical Colors in z 8 Galaxies from GREATS: Very Young Stellar Populations at 650 Myr of Cosmic Time
DOI: 10.3847/1538-4357/ac3de7 Bibcode: 2022ApJ...927...48S

Illingworth, Garth D.; Labbé, Ivo; van Dokkum, Pieter +4 more

Deep rest-optical observations are required to accurately constrain the stellar populations of z ~ 8 galaxies. Due to significant limitations in the availability of such data for statistically complete samples, observational results have been limited to modest numbers of bright or lensed sources. To revolutionize the present characterization of z …

2022 The Astrophysical Journal
eHST 35
First eROSITA study of nearby M dwarfs and the rotation-activity relation in combination with TESS
DOI: 10.1051/0004-6361/202141617 Bibcode: 2022A&A...661A..29M

Salvato, M.; Wolf, J.; Stelzer, B. +3 more

We present the first results with the ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Russian Spektrum-Roentgen-Gamma mission, and we combine the new X-ray data with observations with the Transiting Exoplanet Survey Satellite (TESS). We used the SUPERBLINK proper motion catalog of nearby M dwarfs as input sample to search fo…

2022 Astronomy and Astrophysics
Gaia 35
Macro and micro structures of pebble-made cometary nuclei reconciled by seasonal evolution
DOI: 10.1038/s41550-022-01625-y Bibcode: 2022NatAs...6..546C

Longobardo, Andrea; Mottola, Stefano; Kappel, David +17 more

Comets evolve due to sublimation of ices embedded inside porous dust, triggering dust emission (that is, erosion) followed by mass loss, mass redistribution and surface modifications. Surface changes were revealed by the Deep Impact and Stardust NExT missions for comet 9P/Tempel 1 (ref. 1), and a full inventory of the processes modifyin…

2022 Nature Astronomy
Rosetta 35
Quasi-periodic Energy Release and Jets at the Base of Solar Coronal Plumes
DOI: 10.3847/1538-4357/ac6c24 Bibcode: 2022ApJ...933...21K

Kumar, Pankaj; Deforest, Craig E.; Karpen, Judith T. +3 more

Coronal plumes are long, ray-like, open structures that have been considered as possible sources of the solar wind. Their origin in the largely unipolar coronal holes has long been a mystery. Earlier spectroscopic and imaging observations revealed blueshifted plasma and propagating disturbances (PDs) in plumes that are widely interpreted in terms …

2022 The Astrophysical Journal
IRIS 35
SN 2009ip after a decade: the luminous blue variable progenitor is now gone
DOI: 10.1093/mnras/stac1669 Bibcode: 2022MNRAS.515...71S

Van Dyk, Schuyler D.; Filippenko, Alexei V.; Smith, Nathan +3 more

We present new Hubble Space Telescope (HST) imaging photometry for the site of the Type IIn supernova (SN) 2009ip taken almost a decade after explosion. The optical source has continued to fade steadily since the SN-like event in 2012. In the F606W filter, which was also used to detect its luminous blue variable (LBV) progenitor 13 yr before the S…

2022 Monthly Notices of the Royal Astronomical Society
eHST 34