Search Publications

Black-hole-triggered star formation in the dwarf galaxy Henize 2-10
DOI: 10.1038/s41586-021-04215-6 Bibcode: 2022Natur.601..329S

Schutte, Zachary; Reines, Amy E.

Black-hole-driven outflows have been observed in some dwarf galaxies with active galactic nuclei1, and probably play a role in heating and expelling gas (thereby suppressing star formation), as they do in larger galaxies2. The extent to which black-hole outflows can trigger star formation in dwarf galaxies is unclear, because…

2022 Nature
eHST 43
The prevalence of galaxy overdensities around UV-luminous Lyman 𝛼 emitters in the Epoch of Reionization
DOI: 10.1093/mnras/stac1908 Bibcode: 2022MNRAS.515.5790L

Laporte, N.; Zitrin, A.; Oesch, P. A. +19 more

Before the end of the Epoch of Reionization, the Hydrogen in the Universe was predominantly neutral. This leads to a strong attenuation of Ly α lines of z ≳ 6 galaxies in the intergalactic medium. Nevertheless, Ly α has been detected up to very high redshifts (z ~ 9) for several especially UV luminous galaxies. Here, we test to what extent the gal…

2022 Monthly Notices of the Royal Astronomical Society
eHST 43
The BAyesian STellar algorithm (BASTA): a fitting tool for stellar studies, asteroseismology, exoplanets, and Galactic archaeology
DOI: 10.1093/mnras/stab2911 Bibcode: 2022MNRAS.509.4344A

Christensen-Dalsgaard, J.; Weiss, A.; Serenelli, A. M. +16 more

We introduce the public version of the BAyesian STellar Algorithm (BASTA), an open-source code written in PYTHON to determine stellar properties based on a set of astrophysical observables. BASTA has been specifically designed to robustly combine large data sets that include asteroseismology, spectroscopy, photometry, and astrometry. We describe t…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 43
The updated BASTI stellar evolution models and isochrones - III. White dwarfs
DOI: 10.1093/mnras/stab3359 Bibcode: 2022MNRAS.509.5197S

Salaris, Maurizio; Cassisi, Santi; Pietrinferni, Adriano +1 more

We present new cooling models for carbon-oxygen white dwarfs (WDs) with both H- and He-atmospheres, covering the whole relevant mass range, to extend our updated BASTI (a Bag of Stellar Tracks and Isochrones) stellar evolution archive. They have been computed using core chemical stratifications obtained from new progenitor calculations, adopting a…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 42
The Gaia-ESO Survey: Membership probabilities for stars in 63 open and 7 globular clusters from 3D kinematics
DOI: 10.1093/mnras/stab3032 Bibcode: 2022MNRAS.509.1664J

Gilmore, G.; Montes, D.; Prada Moroni, P. G. +26 more

Spectroscopy from the final internal data release of the Gaia-ESO Survey (GES) has been combined with Gaia EDR3 to assign membership probabilities to targets observed towards 63 Galactic open clusters and 7 globular clusters. The membership probabilities are based chiefly on maximum likelihood modelling of the 3D kinematics of the targets, separat…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 42
Hot subdwarfs in close binaries observed from space. I. Orbital, atmospheric, and absolute parameters, and the nature of their companions
DOI: 10.1051/0004-6361/202244214 Bibcode: 2022A&A...666A.182S

Geier, S.; Pelisoli, I.; Schaffenroth, V. +2 more

Context. About a third of the hot subdwarfs of spectral type B (sdBs), which are mostly core-helium-burning objects on the extreme horizontal branch, are found in close binaries with cool, low-mass stellar, substellar, or white dwarf companions. They can show light variations due to different phenomena.
Aims: Many hot subdwarfs now have space…

2022 Astronomy and Astrophysics
Gaia 42
Exploring the Sgr-Milky Way-disk Interaction Using High-resolution N-body Simulations
DOI: 10.3847/1538-4357/ac5021 Bibcode: 2022ApJ...927..131B

Bovy, Jo; Hunt, Jason A. S.; Bennett, Morgan

The ongoing merger of the Sagittarius (Sgr) dwarf galaxy with the Milky Way is believed to strongly affect the dynamics of the Milky Way's disk. We present a suite of 13 N-body simulations, with 500 million-1 billion particles, modeling the interaction between the Sgr dwarf galaxy and the Galactic disk. To quantify the perturbation to the disk's s…

2022 The Astrophysical Journal
Gaia 42
TESS asteroseismology of the Kepler red giants
DOI: 10.1093/mnras/stac414 Bibcode: 2022MNRAS.512.1677S

Huber, Daniel; García, Rafael A.; Saunders, Nicholas +11 more

Red giant asteroseismology can provide valuable information for studying the Galaxy as demonstrated by space missions like CoRoT and Kepler. However, previous observations have been limited to small data sets and fields of view. The TESS mission provides far larger samples and, for the first time, the opportunity to perform asteroseimic inference …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 42
The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z = 3.5
DOI: 10.1093/mnras/stac1067 Bibcode: 2022MNRAS.513.3510B

Schaerer, D.; Cullen, F.; McLure, R. J. +20 more

We present a study designed to measure the average Lyman-continuum escape fraction (⟨fesc⟩) of star-forming galaxies at z ≃ 3.5. We assemble a sample of 148 galaxies from the VANDELS spectroscopic survey at 3.35 ≤ zspec ≤ 3.95, selected to minimize line-of-sight contamination of their photometry. For this sample, we use ultra…

2022 Monthly Notices of the Royal Astronomical Society
eHST 42
Abundant ammonium hydrosulphide embedded in cometary dust grains
DOI: 10.1093/mnras/stac2440 Bibcode: 2022MNRAS.516.3900A

Altwegg, K.; Fuselier, S. A.; Rubin, M. +7 more

Ammonium hydrosulphide has long since been postulated to exist at least in certain layers of the giant planets. Its radiation products may be the reason for the red colour seen on Jupiter. Several ammonium salts, the products of NH3, and an acid have previously been detected at comet 67P/Churyumov-Gerasimenko. The acid H2S is…

2022 Monthly Notices of the Royal Astronomical Society
Rosetta 42