Search Publications

Hot exozodiacal dust: an exocometary origin?
DOI: 10.1051/0004-6361/201935250 Bibcode: 2019A&A...626A...2S

Augereau, J. -C.; Sezestre, É.; Thébault, P.

Context. Near- and mid-infrared interferometric observations have revealed populations of hot and warm dust grains populating the inner regions of extrasolar planetary systems. These are known as exozodiacal dust clouds, or exozodis, reflecting the similarity with the solar system's zodiacal cloud. Radiative transfer models have constrained the du…

2019 Astronomy and Astrophysics
Gaia 18
Neutral carbon and highly excited CO in a massive star-forming main sequence galaxy at z = 2.2
DOI: 10.1051/0004-6361/201935148 Bibcode: 2019A&A...628A.104B

Daddi, Emanuele; Aravena, Manuel; Decarli, Roberto +5 more

We used the Plateau De Bure Interferometer to observe multiple CO and neutral carbon transitions in a z = 2.2 main sequence disk galaxy, BX610. Our observation of CO(7-6), CO(4-3), and both far-infrared (FIR) [CI] lines complements previous observations of Hα and low-J CO, and reveals a galaxy that is vigorously forming stars with UV fields (Log(G…

2019 Astronomy and Astrophysics
eHST 18
A Closer Look at Some Gas-phase Depletions in the ISM: Trends for O, Ge, and Kr versus {F}_{* }, f(H2), and Starlight Intensity
DOI: 10.3847/1538-4357/aafe81 Bibcode: 2019ApJ...872...55J

Jenkins, Edward B.

In a survey of archived ultraviolet spectra of 100 stars recorded by the echelle spectrograph of the Space Telescope Imaging Spectrograph on the Hubble Space Telescope, we measure the strengths of the weak absorption features of O I, Ge II, and Kr I in the interstellar medium. Our objective is to undertake an investigation that goes beyond earlier…

2019 The Astrophysical Journal
eHST 18
Compositional variations of Titan's impact craters indicates active surface erosion
DOI: 10.1016/j.icarus.2018.12.007 Bibcode: 2019Icar..321..508W

Janssen, M. A.; Cassini Radar Team; Werynski, A. +2 more

Titan, the only moon in the solar system with a considerable atmosphere, is host to a variety of exogenic processes that shape its surface. These processes form features that are quite similar to features on Earth, including sand dunes, rivers, and lakes. The combination of a thick atmosphere and active surface processes also leads to a scarcity o…

2019 Icarus
Cassini 18
The water line emission and ortho-to-para ratio in the Orion Bar photon-dominated region
DOI: 10.1051/0004-6361/201935402 Bibcode: 2019A&A...632A...8P

Le Petit, F.; Roueff, E.; Lis, D. C. +2 more

Context. The ortho-to-para ratio (OPR) of water in the interstellar medium (ISM) is often assumed to be related to the formation temperature of water molecules, making it a potentially interesting tracer of the thermal history of interstellar gas.
Aims: A very low OPR of 0.1-0.5 was previously reported in the Orion Bar photon-dominated region…

2019 Astronomy and Astrophysics
Herschel 18
Interaction of SN Ib 2004dk with a Previously Expelled Envelope
DOI: 10.3847/1538-4357/ab3e36 Bibcode: 2019ApJ...883..120P

Wheeler, J. Craig; Silverman, Jeffrey M.; Pooley, David +7 more

The interaction between the expanding supernova (SN) ejecta with the circumstellar material (CSM) that was expelled from the progenitor prior to explosion is a long-sought phenomenon, yet observational evidence is scarce. Here we confirm a new example: SN 2004dk, originally a hydrogen-poor, helium-rich Type Ib SN that reappeared as a strong {{H}}α…

2019 The Astrophysical Journal
XMM-Newton 18
Numerical Algorithm for Detecting Ion Diffusion Regions in the Geomagnetic Tail With Applications to MMS Tail Season 1 May to 30 September 2017
DOI: 10.1029/2018JA026429 Bibcode: 2019JGRA..124.6487R

Farrugia, C. J.; Torbert, R. B.; Rogers, A. J.

We present a numerical algorithm to identify ion diffusion regions (IDRs) in the geomagnetic tail and test its applicability. We use five criteria applied in three stages. (i) correlated reversals (within 90 s) of Vx and Bz (at least 2 nT about 0; geocentric solar magnetospheric coordinates); (ii) detection of Hall electric a…

2019 Journal of Geophysical Research (Space Physics)
Cluster 18
Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1. IV. Properties of quiescent galaxies on the stellar mass-size plane
DOI: 10.1051/0004-6361/201935257 Bibcode: 2019A&A...631A.158D

Cenarro, A. J.; López-Sanjuan, C.; Perea, J. +7 more


Aims: We perform a comprehensive study of the stellar population properties (formation epoch, age, metallicity, and extinction) of quiescent galaxies as a function of size and stellar mass to constrain the physical mechanism governing the stellar mass assembly and the likely evolutive scenarios that explain their growth in size.
Methods:…

2019 Astronomy and Astrophysics
eHST 18
The blue straggler population of the old open cluster Berkeley 17
DOI: 10.1051/0004-6361/201834449 Bibcode: 2019A&A...624A..26B

Chen, W. P.; Beccari, Giacomo; Vaidya, Kaushar +1 more

Context. Blue straggler stars (BSSs) are observed in Galactic globular clusters and old open clusters. The radial distribution of BSSs has been used to diagnose the dynamical evolution of globular clusters. For the first time, with a reliable sample of BSSs identified with Gaia DR2, we conduct such an analysis for an open cluster.
Aims: We ai…

2019 Astronomy and Astrophysics
Gaia 18
Detection and Classification of Supernovae Beyond z ∼ 2 Redshift with the James Webb Space Telescope
DOI: 10.3847/1538-4357/ab0a73 Bibcode: 2019ApJ...874..158R

Vinkó, József; Regős, Enikő

Future time-domain surveys for transient events in the near- and midinfrared bands will significantly extend our understanding about the physics of the early universe. In this paper we study the implications of a deep (∼27 mag), long-term (∼3 yr), observationally inexpensive survey with the James Webb Space Telescope (JWST) within its Continuous V…

2019 The Astrophysical Journal
eHST 18