Zobrazeno 1 - 10
of 54
pro vyhledávání: '"Benedettini, Milena"'
Autor:
Kirk, Jason, Ward-Thompson, Derek, Di Francesco, James, André, Philippe, Bresnahan, David, Könyves, Vera, Marsh, Kenneth, Griffin, Matt, Schneider, Nicola, Men'shchikov, A., Palmeirim, Pedro, Bontemps, Sylvain, Arzoumanian, Doris, Benedettini, Milena, Pezzuto, Stefania
We present a catalogue of dense cores and filaments in a $3.8^{\circ}\times2.4^{\circ}$ field around the TMC1 region of the Taurus Molecular Cloud. The catalogue was created using photometric data from the Herschel SPIRE and PACS instruments in the 7
Externí odkaz:
http://arxiv.org/abs/2407.01233
Autor:
Hunter, Glen H., Sormani, Mattia C., Beckmann, Jan P., Vasiliev, Eugene, Glover, Simon C. O., Klessen, Ralf S., Soler, Juan D., Brucy, Noé, Girichidis, Philipp, Göller, Junia, Ohlin, Loke, Tress, Robin, Molinari, Sergio, Gerhard, Ortwin, Benedettini, Milena, Smith, Rowan, Hennebelle, Patrick, Testi, Leonardo
Obtaining reliable distance estimates to gas clouds within the Milky Way is challenging in the absence of certain tracers. The kinematic distance approach has been used as an alternative, derived from the assumption of circular trajectories around th
Externí odkaz:
http://arxiv.org/abs/2403.18000
Autor:
Colman, Tine, Brucy, Noé, Girichidis, Philipp, Glover, Simon C. O, Benedettini, Milena, Soler, Juan D., Tress, Robin G., Traficante, Alessio, Hennebelle, Patrick, Klessen, Ralf S., Molinari, Sergio, Miville-Deschênes, Marc-Antoine
Publikováno v:
A&A 686, A155 (2024)
Molecular clouds (MC) are structures of dense gas in the interstellar medium (ISM), that extend from ten to a few hundred parsecs and form the main gas reservoir available for star formation. Hydrodynamical simulations of varying complexity are a pro
Externí odkaz:
http://arxiv.org/abs/2403.00512
Autor:
Di Francesco, James, Keown, Jared, Fallscheer, Cassandra, André, Philippe, Ladjelate, Bilal, Könyves, Vera, Men'shchikov, Alexander, Stephens-Whale, Shaun, Nguyen-Luong, Quang, Martin, Peter, Sadavoy, Sarah, Pezzuto, Stefano, Fiorellino, Eleonora, Benedettini, Milena, Schneider, Nicola, Bontemps, Sylvain, Arzoumanian, Doris, Palmeirim, Pedro, Kirk, Jason M., Ward-Thompson, Derek
We present Herschel SPIRE and PACS maps of the Cepheus Flare clouds L1157, L1172, L1228, L1241, and L1251, observed by the Herschel Gould Belt Survey (HGBS) of nearby star-forming molecular clouds. Through modified blackbody fits to the SPIRE and PAC
Externí odkaz:
http://arxiv.org/abs/2010.09894
Autor:
Ladjelate, Bilal, André, Philippe, Könyves, Vera, Ward-Thompson, Derek, Men'shchikov, Alexander, Bracco, Andrea, Palmeirim, Pedro, Roy, Arabindo, Shimajiri, Yoshito, Kirk, Jason M., Arzoumanian, Doris, Benedettini, Milena, Di Francesco, James, Fiorellino, Eleonora, Schneider, Nicola, Pezzuto, Stefano
Publikováno v:
A&A 638, A74 (2020)
Herschel observations of nearby clouds in the Gould Belt support a paradigm for low-mass star formation, starting with the generation of molecular filaments, followed by filament fragmentation, and the concentration of mass into self-gravitating pres
Externí odkaz:
http://arxiv.org/abs/2001.11036
Autor:
Holdship, Jonathan, Jimenez-Serra, Izaskun, Viti, Serena, Codella, Claudio, Benedettini, Milena, Fontani, Francesco, Podio, Linda, Tafalla, Mario, Bachiller, Rafael, Ceccarelli, Cecilia
The main carrier of sulfur in dense clouds, where it is depleted from the gas phase, remains a mystery. Shock waves in young molecular outflows disrupt the ice mantles and allow us to directly probe the material that is ejected into the gas phase. A
Externí odkaz:
http://arxiv.org/abs/1904.10895
Autor:
Baldeschi, Adriano, Elia, Davide, Molinari, Sergio, Pezzuto, Stefano, Schisano, Eugenio, Gatti, Marco, Serra, Andrea, Benedettini, Milena, Di Giorgio, Anna Maria, Liu, John Scige, Merello, Manuel
The degradation of spatial resolution in star-forming regions observed at large distances ($d\gtrsim1$ kpc) with Herschel,can lead to estimates of the physical parameters of the detected compact sources (clumps) which do not necessarily mirror the pr
Externí odkaz:
http://arxiv.org/abs/1701.08035
Autor:
Holdship, Jonathan, Viti, Serena, Jimenez-Serra, Izaskun, Lefloch, Bertrand, Codella, Claudio, Podio, Linda, Benedettini, Milena, Fontani, Francesco, Bachiller, Rafael, Tafalla, Mario, Ceccarelli, Cecilia
Sulfur-bearing molecules are highly reactive in the gas phase of the ISM. However, the form in which most of the sulfur is locked onto interstellar dust grains is unknown. By taking advantage of the short time-scales of shocks in young molecular outf
Externí odkaz:
http://arxiv.org/abs/1608.01983
Autor:
Molinari, Sergio, Noriega-Crespo, Alberto, Bally, John, Moore, Toby, Elia, Davide, Schisano, Eugenio, Plume, Rene, Swinyard, Bruce, Di Giorgio, Anna Maria, Pezzuto, Stefano, Benedettini, Milena, Testi, Leonardo
We use the Herschel Hi-GAL survey data to study the spatial distribution in Galactic longitude and latitude of the interstellar medium and of dense, star-forming clumps in the inner Galaxy. The peak position and width of the latitude distribution of
Externí odkaz:
http://arxiv.org/abs/1511.06300
Autor:
Riccio, Giuseppe, Cavuoti, Stefano, Schisano, Eugenio, Brescia, Massimo, Mercurio, Amata, Elia, Davide, Benedettini, Milena, Pezzuto, Stefano, Molinari, Sergio, Di Giorgio, Anna Maria
We present an innovative method called FilExSeC (Filaments Extraction, Selection and Classification), a data mining tool developed to investigate the possibility to refine and optimize the shape reconstruction of filamentary structures detected with
Externí odkaz:
http://arxiv.org/abs/1505.06621