4 results
Search Results
Now showing 1 - 4 of 4
- ItemThe Abundance of S-Process Elements: Temporal and Spatial Trends from Open Cluster Observations(Basel : MDPI, 2022) Magrini, Laura; Vázquez, Carlos Viscasillas; Casali, Giada; Baratella, Martina; D’Orazi, Valentina; Spina, Lorenzo; Randich, Sofia; Cristallo, Sergio; Vescovi, DiegoSpectroscopic observations of stars belonging to open clusters, with well-determined ages and distances, are a unique tool for constraining stellar evolution, nucleosynthesis, mixing processes, and, ultimately, Galactic chemical evolution. Abundances of slow (s) process neutron capture elements in stars that retain their initial surface composition open a window into the processes that generated them. In particular, they give us information on their main site of production, i.e., the low-and intermediate-mass Asymptotic Giant Branch (AGB) stars. In the present work, we review some observational results obtained during the last decade that contributed to a better understanding of the AGB phase: the growth of s-process abundances at recent epochs, i.e., in the youngest stellar populations; the different relations between age and [s/Fe] in distinct regions of the disc; and finally the use of s-process abundances combined with those of α elements, [s/α], to estimate stellar ages. We revise some implications that these observations had both on stellar and Galactic evolution, and on our ability to infer stellar ages.
- ItemThe Complex Behaviour of s-Process Element Abundances at Young Ages(Basel : MDPI, 2022) D’Orazi, Valentina; Baratella, Martina; Lugaro, Maria; Magrini, Laura; Pignatari, MarcoOpen clusters appear as simple objects in many respects, with a high degree of homogeneity in their (initial) chemical composition, and the typical solar-scaled abundance pattern that they exhibit for the majority of the chemical species. The striking singularity is represented by heavy elements produced from the slow process of the neutron-capture reactions. In particular, young open clusters (ages less than a few hundred Myr) give rise to the so-called barium puzzle: that is an extreme enhancement in their [Be/Fe] ratios, up to a factor of four of the solar value, which is not followed by other nearby s-process elements (e.g., lanthanum and cerium). The definite explanation for such a peculiar trend is still wanting, as many different solutions have been envisaged. We review the status of this field and present our new results on young open clusters and the pre-main sequence star RZ Piscium.
- ItemSpace Photometry with BRITE-Constellation(Basel : MDPI, 2021) Weiss, Werner; Zwintz, Konstanze; Kuschnig, Rainer; Handler, Gerald; Moffat, Anthony; Baade, Dietrich; Bowman, Dominic; Granzer, Thomas; Kallinger, Thomas; Koudelka, Otto; Lovekin, Catherine; Neiner, Coralie; Pablo, Herbert; Pigulski, Andrzej; Popowicz, Adam; Ramiaramanantsoa, Tahina; Rucinski, Slavek; Strassmeier, Klaus; Wade, GreggBRITE-Constellation is devoted to high-precision optical photometric monitoring of bright stars, distributed all over the Milky Way, in red and/or blue passbands. Photometry from space avoids the turbulent and absorbing terrestrial atmosphere and allows for very long and continuous observing runs with high time resolution and thus provides the data necessary for understanding various processes inside stars (e.g., asteroseismology) and in their immediate environment. While the first astronomical observations from space focused on the spectral regions not accessible from the ground it soon became obvious around 1970 that avoiding the turbulent terrestrial atmosphere significantly improved the accuracy of photometry and satellites explicitly dedicated to high-quality photometry were launched. A perfect example is BRITE-Constellation, which is the result of a very successful cooperation between Austria, Canada and Poland. Research highlights for targets distributed nearly over the entire HRD are presented, but focus primarily on massive and hot stars.
- ItemSearching for Magnetospheres around Herbig Ae/Be Stars(Basel : MDPI, 2021) Pogodin, Mikhail; Drake, Natalia; Beskrovnaya, Nina; Pavlovskiy, Sergei; Hubrig, Swetlana; Schöller, Markus; Järvinen, Silva; Kozlova, Olesya; Alekseev, IlyaWe describe four different approaches for the detection of magnetospheric accretion among Herbig Ae/Be stars with accretion disks. Studies of several unique objects have been carried out. One of the objects is the Herbig Ae star HD 101412 with a comparatively strong magnetic field. The second is the early-type Herbig B6e star HD 259431. The existence of a magnetosphere in these objects was not recognized earlier. In both cases, a periodicity in the variation of some line parameters, originating near the region of the disk/star interaction, has been found. The third object is the young binary system HD 104237, hosting a Herbig Ae star and a T Tauri star. Based on the discovery of periodic variations of equivalent widths of atmospheric lines in the spectrum of the primary, we have concluded that the surface of the star is spotted. Comparing our result with an earlier one, we argue that these spots can be connected with the infall of material from the disk onto the stellar surface through a magnetosphere. The fourth example is the Herbig Ae/Be star HD 37806. Signatures of magnetospheric accretion in this object have been identified using a different method. They were inferred from the short-term variability of the He I λ5876 line profile forming in the region of the disk/star interaction.