Search Publications

Current Challenges in Cepheid Distance Calibrations Using Gaia Early Data Release 3
DOI: 10.3847/1538-4357/ac479e Bibcode: 2022ApJ...927....8O

Madore, Barry F.; Freedman, Wendy L.; Lee, Abigail J. +1 more

Using parallaxes from Gaia Early Data Release 3 (EDR3), we determine multi-wavelength BVI c , JHK s , and [3.6] and [4.5] micron absolute magnitudes for 37 nearby Milky Way Cepheids, covering the period range between 5 and 60 days. We apply these period-luminosity relations to Cepheids in the Large and Small Magellanic Clou…

2022 The Astrophysical Journal
Gaia 23
AGN impact on the molecular gas in galactic centres as probed by CO lines
DOI: 10.1093/mnras/stac313 Bibcode: 2022MNRAS.512..686E

Vallini, Livia; Mingozzi, Matilde; Vignali, Cristian +5 more

We present a detailed analysis of the X-ray, infrared, and carbon monoxide (CO) emission for a sample of 35 local (z ≤ 0.15), active (LX ≥ 1042 erg s-1) galaxies. Our goal is to infer the contribution of far-ultraviolet (FUV) radiation from star formation (SF), and X-ray radiation from the active galactic nuclei (A…

2022 Monthly Notices of the Royal Astronomical Society
Herschel eHST 23
Turbulence in the Outer Heliosphere
DOI: 10.1007/s11214-022-00914-2 Bibcode: 2022SSRv..218...50F

Zank, Gary P.; Adhikari, Laxman; Zhao, Lingling +9 more

The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their interaction is governed by complex physical processes and creates heliospheric regions with significantly different properties in terms of particle populations, bulk flow and turbulence. Our knowledge of the solar wind turbulence nature and dynamics mostly relies o…

2022 Space Science Reviews
Ulysses 23
TOI-3884 b: A rare 6-RE planet that transits a low-mass star with a giant and likely polar spot
DOI: 10.1051/0004-6361/202244791 Bibcode: 2022A&A...667L..11A

Bouchy, F.; Bonfils, X.; Ciardi, D. R. +19 more

The Transiting Exoplanet Survey Satellite mission identified a deep and asymmetric transit-like signal with a periodicity of 4.5 days orbiting the M4 dwarf star TOI-3884. The signal has been confirmed by follow-up observations collected by the ExTrA facility and Las Cumbres Observatory Global Telescope, which reveal that the transit is chromatic. …

2022 Astronomy and Astrophysics
Gaia 23
Detection of 2460 double-lined spectroscopic binary candidates in the LAMOST-MRS using projected rotational velocities and a binary spectral model
DOI: 10.1093/mnras/stac2513 Bibcode: 2022MNRAS.517..356K

Han, Zhanwen; Kovalev, Mikhail; Chen, Xuefei

We present a new method for the detection of double-lined spectroscopic binaries (SB2s) using Vsin i values from spectral fits. The method is tested on synthetic and real spectra from the Large Sky Area Multi-Object fiber Spectroscopic Telescope Medium Resolution Survey. It can reliably detect SB2 candidates for double-lined binaries with $V \sin …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22
Transient acceleration events in LISA Pathfinder data: Properties and possible physical origin
DOI: 10.1103/PhysRevD.106.062001 Bibcode: 2022PhRvD.106f2001A

Mendes, L.; Russano, G.; Nofrarias, M. +79 more

We present an in depth analysis of the transient events, or glitches, detected at a rate of about one per day in the differential acceleration data of LISA Pathfinder. We show that these glitches fall in two rather distinct categories: fast transients in the interferometric motion readout on one side, and true force transient events on the other. …

2022 Physical Review D
LISAPathfinder 22
A solar coronal loop in a box: Energy generation and heating
DOI: 10.1051/0004-6361/202141451 Bibcode: 2022A&A...658A..45B

Peter, H.; Chitta, L. P.; Solanki, S. K. +4 more

Context. Coronal loops are the basic building block of the upper solar atmosphere as seen in the extreme UV and X-rays. Comprehending how these are energized, structured, and evolve is key to understanding stellar coronae.
Aims: Here we investigate how the energy to heat the loop is generated by photospheric magneto-convection, transported in…

2022 Astronomy and Astrophysics
Hinode 22
Wide Twin Binaries are Extremely Eccentric: Evidence of Twin Binary Formation in Circumbinary Disks
DOI: 10.3847/2041-8213/ac7c70 Bibcode: 2022ApJ...933L..32H

Ting, Yuan-Sen; Rix, Hans-Walter; Zakamska, Nadia L. +3 more

The Gaia mission recently revealed an excess population of equal-mass "twin" wide binaries, with mass ratio q ≳ 0.95, extending to separations of at least 1000 au. The origin of this population is an enigma: Twin binaries are thought to form via correlated accretion in circumbinary disks, but the typical observed protostellar disks have radii of ~…

2022 The Astrophysical Journal
Gaia 22
An INTEGRAL/SPI view of reticulum II: particle dark matter and primordial black holes limits in the MeV range
DOI: 10.1093/mnras/stac008 Bibcode: 2022MNRAS.511..914S

Calore, Francesca; Vincent, Aaron C.; Diehl, Roland +4 more

Reticulum II (Ret II) is a satellite galaxy of the Milky Way (MW) and presents a prime target to investigate the nature of dark matter (DM) because of its high mass-to-light ratio. We evaluate a dedicated INTEGRAL observation campaign data set to obtain γ-ray fluxes from Ret II and compare those with expectations from DM. Ret II is not detected in…

2022 Monthly Notices of the Royal Astronomical Society
INTEGRAL 22
Contribution of Gaia Sausage to the Galactic Stellar Halo Revealed by K Giants and Blue Horizontal Branch Stars from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, Sloan Digital Sky Survey, and Gaia
DOI: 10.3847/1538-4357/ac31ac Bibcode: 2022ApJ...924...23W

Bird, Sarah A.; Zhao, Gang; Yang, Chengqun +2 more

We explore the contribution of the Gaia Sausage to the stellar halo of the Milky Way by making use of a Gaussian mixture model (GMM) and applying it to halo star samples of Large Sky Area Multi-Object Fiber Spectroscopic Telescope K giants, Sloan Extension for Galactic Understanding and Exploration K giants, and Sloan Digital Sky Survey blue horiz…

2022 The Astrophysical Journal
Gaia 22