Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Silvia Raso"'
Autor:
Sebastian Kamann, Andrea Bellini, Giacomo Beccari, Michele Bellazzini, Silvia Raso, Emanuele Dalessandro, Enrico Vesperini
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 506:813-823
We present a detailed 3D kinematic analysis of the central regions ($R
13 pages, 12 figures, 2 tables; accepted for publication in MNRAS
13 pages, 12 figures, 2 tables; accepted for publication in MNRAS
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 500, 2012-2019. Oxford University Press
We present $\it{Hubble}$ $\it{Space}$ $\it{Telescope}$ proper motions in the direction of the star cluster NGC$\,$419 in the Small Magellanic Cloud. Because of the high precision of our measurements, for the first time it is possible to resolve the c
Autor:
Mattia Libralato, Francesco R. Ferraro, Giampaolo Piotto, Emanuele Dalessandro, M. Cadelano, Silvia Raso, Jay Anderson, Barbara Lanzoni, Andrea Bellini, Sangmo Tony Sohn, C. Pallanca
We constructed a Hubble Space Telescope (HST) astro-photometric catalog of the central region of the Galactic globular cluster NGC 1261. This catalog, complemented with Gaia DR2 data sampling the external regions, has been used to estimate the struct
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f087120a961fd54580135ff1c8acec3a
http://hdl.handle.net/11585/802630
http://hdl.handle.net/11585/802630
Autor:
Paola Focardi, C. Pallanca, Barbara Lanzoni, Giacomo Beccari, Emanuele Dalessandro, Alessio Mucciarelli, Francesco R. Ferraro, M. Cadelano, Silvia Raso
We used resolved star counts from Hubble Space Telescope images to determine the center of gravity and the projected density profiles of 6 old globular clusters in the Large Magellanic Cloud (LMC), namely NGC 1466, NGC 1841, NGC 1898, NGC 2210, NGC 2
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3d1b9511409b20608b08b4d7eda2a05e
http://arxiv.org/abs/1911.01928
http://arxiv.org/abs/1911.01928
Publikováno v:
The Astrophysical Journal
We used optical images acquired with the UVIS channel of the Wide Field Camera 3 on board of the Hubble Space Telescope to construct the first high-resolution extinction map in the direction of NGC 6440, a globular cluster located in the bulge of our
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::433fddc6ded97b656d1344fb5bc8048f
http://arxiv.org/abs/1908.09708
http://arxiv.org/abs/1908.09708
Autor:
Francesco R. Ferraro, Alison Sills, Giacomo Beccari, Jongsuk Hong, Enrico Vesperini, Barbara Lanzoni, Emanuele Dalessandro, Andrea Dieball, Silvia Raso, Christian Knigge, Livia Origlia
In this paper we report on the discovery of a double blue straggler star (BSS) sequence in the core of the core-collapsed cluster M15 (NGC 7078). We performed a detailed photometric analysis of the extremely dense core of the cluster using a set of i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fe4a506ad59c046f6e9d1b68925ffd23
http://arxiv.org/abs/1903.11113
http://arxiv.org/abs/1903.11113
Autor:
Francesco R. Ferraro, C. Pallanca, Barbara Lanzoni, M. Cadelano, Giacomo Beccari, Emanuele Dalessandro, Alessio Mucciarelli, Silvia Raso
The distribution of size as a function of age observed for star clusters in the Large Magellanic Cloud (LMC) is very puzzling: young clusters are all compact, while the oldest systems show both small and large sizes. It is commonly interpreted as due
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0927e36d246ceb3a7318bbbf4af59ee4
http://hdl.handle.net/11585/725401
http://hdl.handle.net/11585/725401
Autor:
Emanuele Dalessandro, Francesco R. Ferraro, Nate Bastian, Barbara Lanzoni, M. Cadelano, Silvia Raso
Li et al. (2018a; Li18a) claimed that the young stellar cluster NGC2173 in the Large Magellanic Cloud (LMC) harbours a bifurcated sequence of blue straggler stars (BSSs), similar to those detected in a few dynamically old globular clusters. However,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4ba3946c8a0e3918ae4c27a4e66d1871
http://hdl.handle.net/20.500.12386/30462
http://hdl.handle.net/20.500.12386/30462
Autor:
Francesco R. Ferraro, Andrea Bellini, Alessio Mucciarelli, Silvia Raso, Barbara Lanzoni, Mattia Libralato, C. Pallanca, Emanuele Dalessandro, Jay Anderson, Livia Origlia
We have constructed the Spectral Energy Distributions (SEDs) of a sample of Blue Straggler Stars (BSSs) in the core of the globular cluster 47 Tucanae, taking advantage of the large set of high resolution images, ranging from the ultraviolet to the n
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e5b240ef19bdc585b1b87c61d7c66def
http://hdl.handle.net/20.500.12386/30460
http://hdl.handle.net/20.500.12386/30460
Autor:
Giampaolo Piotto, C. Pallanca, Giacomo Beccari, Sergio Ortolani, Domenico Nardiello, Enrico Vesperini, Emanuele Dalessandro, Alvio Renzini, Mattia Libralato, Luigi R. Bedin, Francesco R. Ferraro, Jay Anderson, Andrea Bellini, R. P. van der Marel, Antonio Aparicio, Barbara Lanzoni, Santi Cassisi, Silvia Raso, Antonino Milone, Maurizio Salaris
Publikováno v:
The Astrophysical Journal
The parameter A+, defined as the area enclosed between the cumulative radial distribution of blue straggler stars (BSSs) and that of a reference population, is a powerful indicator of the level of BSS central segregation. As part of the Hubble Space