Search Publications

Forbidden hugs in pandemic times. I. Luminous red nova AT 2019zhd, a new merger in M 31
DOI: 10.1051/0004-6361/202039952 Bibcode: 2021A&A...646A.119P

Lundqvist, P.; Rest, A.; Munari, U. +20 more

We present the follow-up campaign of the luminous red nova (LRN) AT 2019zhd, the third event of this class observed in M 31. The object was followed by several sky surveys for about five months before the outburst, during which it showed a slow luminosity rise. In this phase, the absolute magnitude ranged from…

2021 Astronomy and Astrophysics
eHST 27
Water Group Exospheres and Surface Interactions on the Moon, Mercury, and Ceres
DOI: 10.1007/s11214-021-00846-3 Bibcode: 2021SSRv..217...74S

Li, Shuai; Wöhler, Christian; Berezhnoy, Alexey A. +7 more

Water ice, abundant in the outer solar system, is volatile in the inner solar system. On the largest airless bodies of the inner solar system (Mercury, the Moon, Ceres), water can be an exospheric species but also occurs in its condensed form. Mercury hosts water ice deposits in permanently shadowed regions near its poles that act as cold traps. W…

2021 Space Science Reviews
Herschel 27
ALMA survey of Lupus class III stars: Early planetesimal belt formation and rapid disc dispersal
DOI: 10.1093/mnras/staa3335 Bibcode: 2021MNRAS.500.4878L

Testi, L.; Tazzari, M.; Williams, J. P. +9 more

Class III stars are those in star forming regions without large non-photospheric infrared emission, suggesting recent dispersal of their protoplanetary discs. We observed 30 class III stars in the 1-3 Myr Lupus region with ALMA at ∼856µm, resulting in four detections that we attribute to circumstellar dust. Inferred dust masses are 0.036-0.0…

2021 Monthly Notices of the Royal Astronomical Society
Gaia Herschel 27
Cloud-by-cloud, multiphase, Bayesian modelling: application to four weak, low-ionization absorbers
DOI: 10.1093/mnras/staa3754 Bibcode: 2021MNRAS.501.2112S

Richter, Philipp; Charlton, Jane C.; Kacprzak, Glenn G. +8 more

We present a new method aimed at improving the efficiency of component by component ionization modelling of intervening quasar absorption-line systems. We carry out cloud-by-cloud, multiphase modelling making use of CLOUDY and Bayesian methods to extract physical properties from an ensemble of absorption profiles. Here, as a demonstration of metho…

2021 Monthly Notices of the Royal Astronomical Society
eHST 27
Circumbinary and circumstellar discs around the eccentric binary IRAS 04158+2805 - a testbed for binary-disc interaction
DOI: 10.1093/mnras/stab2179 Bibcode: 2021MNRAS.507.1157R

Duchêne, Gaspard; Ménard, François; Stapelfeldt, Karl +10 more

IRAS 04158+2805 has long been thought to be a very low mass T-Tauri star (VLMS) surrounded by a nearly edge-on, extremely large disc. Recent observations revealed that this source hosts a binary surrounded by an extended circumbinary disc with a central dust cavity. In this paper, we combine ALMA multiwavelength observations of continuum and

2021 Monthly Notices of the Royal Astronomical Society
Gaia 27
High tide: a systematic search for ellipsoidal variables in ASAS-SN
DOI: 10.1093/mnras/stab2126 Bibcode: 2021MNRAS.507..104R

Kochanek, C. S.; Stanek, K. Z.; Thompson, Todd A. +5 more

The majority of non-merging stellar mass black holes are discovered by observing high energy emission from accretion processes. Here, we pursue the large, but still mostly unstudied population of non-interacting black holes and neutron stars by searching for the tidally induced ellipsoidal variability of their stellar companions. We start from a s…

2021 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 27
Asteroid absolute magnitudes and phase curve parameters from Gaia photometry
DOI: 10.1051/0004-6361/202039796 Bibcode: 2021A&A...649A..98M

Cellino, A.; Muinonen, K.; Penttilä, A. +2 more


Aims: We perform light curve inversion for 491 asteroids to retrieve phase curve parameters, rotation periods, pole longitudes and latitudes, and convex and triaxial ellipsoid shapes by using the sparse photometric observations from Gaia Data Release 2 and the dense ground-based observations from the DAMIT database. We develop a method for th…

2021 Astronomy and Astrophysics
Gaia 27
Bird's eye view of molecular clouds in the Milky Way. I. Column density and star formation from sub-parsec to kiloparsec scales
DOI: 10.1051/0004-6361/202040021 Bibcode: 2021A&A...653A..63S

Kainulainen, Jouni; Spilker, Andri; Orkisz, Jan

Context. Describing how the properties of the interstellar medium are combined across various size scales is crucial for understanding star formation scaling laws and connecting Galactic and extragalactic data of molecular clouds.
Aims: We describe how the statistical structure of the clouds and its connection to star formation changes from s…

2021 Astronomy and Astrophysics
Herschel 26
On the Use of Field RR Lyrae As Galactic Probes: IV. New Insights Into and Around the Oosterhoff Dichotomy
DOI: 10.3847/1538-4357/ac1115 Bibcode: 2021ApJ...919..118F

Salaris, M.; Lemasle, B.; Zoccali, M. +30 more

We discuss the largest and most homogeneous spectroscopic data set of field RR Lyrae variables (RRLs) available to date. We estimated abundances using both high-resolution and low-resolution (ΔS method) spectra for fundamental (RRab) and first overtone (RRc) RRLs. The iron abundances for 7941 RRLs were supplemented with similar estimates that are …

2021 The Astrophysical Journal
Gaia 26
Solo dwarfs - III. Exploring the orbital origins of isolated Local Group galaxies with Gaia Data Release 2
DOI: 10.1093/mnras/staa3740 Bibcode: 2021MNRAS.501.2363M

Lewis, Geraint F.; McConnachie, Alan W.; Venn, Kim A. +4 more

We measure systemic proper motions for distant dwarf galaxies in the Local Group and investigate if these isolated galaxies have ever had an interaction with the Milky Way or M31. We cross-match photometry of isolated, star-forming, dwarf galaxies in the Local Group, taken as part of the Solo survey, with astrometric measurements from Gaia Data Re…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 26