Zobrazeno 1 - 10
of 165
pro vyhledávání: '"Fontani, Francesco"'
Autor:
Fontani, Francesco
The chemistry of phosphorus (31P) in space is particularly significant due to the key role it plays in biochemistry on Earth. Utilising radio and infrared spectroscopic observations, several key phosphorus-containing molecules have been detected in i
Externí odkaz:
http://arxiv.org/abs/2407.19006
Autor:
Chahine, Layal, Ceccarelli, Cecilia, De Simone, Marta, Chandler, Claire J., Codella, Claudio, Podio, Linda, López-Sepulcre, Ana, Sakai, Nami, Loinard, Laurent, Bouvier, Mathilde, Caselli, Paola, Vastel, Charlotte, Bianchi, Eleonora, Cuello, Nicolás, Fontani, Francesco, Johnstone, Doug, Sabatini, Giovanni, Hanawa, Tomoyuki, Zhang, Ziwei E., Aikawa, Yuri, Busquet, Gemma, Caux, Emmanuel, Durán, Aurore, Herbst, Eric, Ménard, François, Segura-Cox, Dominique, Svodoba, Brian, Balucani, Nadia, Charnley, Steven, Dulieu, François, Evans, Lucy, Fedele, Davide, Feng, Siyi, Hama, Tetsuya, Hirota, Tomoya, Isella, Andrea, Jímenez-Serra, Izaskun, Lefloch, Bertrand, Maud, Luke T., Maureira, María José, Miotello, Anna, Moellenbrock, George, Nomura, Hideko, Oba, Yasuhiro, Ohashi, Satoshi, Okoda, Yuki, Oya, Yoko, Pineda, Jaime, Rimola, Albert, Sakai, Takeshi, Shirley, Yancy, Testi, Leonardo, Viti, Serena, Watanabe, Naoki, Watanabe, Yoshimasa, Zhang, Yichen, Yamamoto, Satoshi
The exploration of outflows in protobinary systems presents a challenging yet crucial endeavour, offering valuable insights into the dynamic interplay between protostars and their evolution. In this study, we examine the morphology and dynamics of je
Externí odkaz:
http://arxiv.org/abs/2405.12735
Autor:
Mainieri, Vincenzo, Anderson, Richard I., Brinchmann, Jarle, Cimatti, Andrea, Ellis, Richard S., Hill, Vanessa, Kneib, Jean-Paul, McLeod, Anna F., Opitom, Cyrielle, Roth, Martin M., Sanchez-Saez, Paula, Smiljanic, Rodolfo, Tolstoy, Eline, Bacon, Roland, Randich, Sofia, Adamo, Angela, Annibali, Francesca, Arevalo, Patricia, Audard, Marc, Barsanti, Stefania, Battaglia, Giuseppina, Aran, Amelia M. Bayo, Belfiore, Francesco, Bellazzini, Michele, Bellini, Emilio, Beltran, Maria Teresa, Berni, Leda, Bianchi, Simone, Biazzo, Katia, Bisero, Sofia, Bisogni, Susanna, Bland-Hawthorn, Joss, Blondin, Stephane, Bodensteiner, Julia, Boffin, Henri M. J., Bonito, Rosaria, Bono, Giuseppe, Bouche, Nicolas F., Bowman, Dominic, Braga, Vittorio F., Bragaglia, Angela, Branchesi, Marica, Brucalassi, Anna, Bryant, Julia J., Bryson, Ian, Busa, Innocenza, Camera, Stefano, Carbone, Carmelita, Casali, Giada, Casali, Mark, Casasola, Viviana, Castro, Norberto, Catelan, Marcio, Cavallo, Lorenzo, Chiappini, Cristina, Cioni, Maria-Rosa, Colless, Matthew, Colzi, Laura, Contarini, Sofia, Couch, Warrick, D'Ammando, Filippo, D., William d'Assignies, D'Orazi, Valentina, da Silva, Ronaldo, Dainotti, Maria Giovanna, Damiani, Francesco, Danielski, Camilla, De Cia, Annalisa, de Jong, Roelof S., Dhawan, Suhail, Dierickx, Philippe, Driver, Simon P., Dupletsa, Ulyana, Escoffier, Stephanie, Escorza, Ana, Fabrizio, Michele, Fiorentino, Giuliana, Fontana, Adriano, Fontani, Francesco, Sanchez, Daniel Forero, Franois, Patrick, Galindo-Guil, Francisco Jose, Gallazzi, Anna Rita, Galli, Daniele, Garcia, Miriam, Garcia-Rojas, Jorge, Garilli, Bianca, Grand, Robert, Guarcello, Mario Giuseppe, Hazra, Nandini, Helmi, Amina, Herrero, Artemio, Iglesias, Daniela, Ilic, Dragana, Irsic, Vid, Ivanov, Valentin D., Izzo, Luca, Jablonka, Pascale, Joachimi, Benjamin, Kakkad, Darshan, Kamann, Sebastian, Koposov, Sergey, Kordopatis, Georges, Kovacevic, Andjelka B., Kraljic, Katarina, Kuncarayakti, Hanindyo, Kwon, Yuna, La Forgia, Fiorangela, Lahav, Ofer, Laigle, Clotilde, Lazzarin, Monica, Leaman, Ryan, Leclercq, Floriane, Lee, Khee-Gan, Lee, David, Lehnert, Matt D., Lira, Paulina, Loffredo, Eleonora, Lucatello, Sara, Magrini, Laura, Maguire, Kate, Mahler, Guillaume, Majidi, Fatemeh Zahra, Malavasi, Nicola, Mannucci, Filippo, Marconi, Marcella, Martin, Nicolas, Marulli, Federico, Massari, Davide, Matsuno, Tadafumi, Mattheee, Jorryt, McGee, Sean, Merc, Jaroslav, Merle, Thibault, Miglio, Andrea, Migliorini, Alessandra, Minchev, Ivan, Minniti, Dante, Miret-Roig, Nuria, Ibero, Ana Monreal, Montano, Federico, Montet, Ben T., Moresco, Michele, Moretti, Chiara, Moscardini, Lauro, Moya, Andres, Mueller, Oliver, Nanayakkara, Themiya, Nicholl, Matt, Nordlander, Thomas, Onori, Francesca, Padovani, Marco, Pala, Anna Francesca, Panda, Swayamtrupta, Pandey-Pommier, Mamta, Pasquini, Luca, Pawlak, Michal, Pessi, Priscila J., Pisani, Alice, Popovic, Lukav C., Prisinzano, Loredana, Raddi, Roberto, Rainer, Monica, Rebassa-Mansergas, Alberto, Richard, Johan, Rigault, Mickael, Rocher, Antoine, Romano, Donatella, Rosati, Piero, Sacco, Germano, Sanchez-Janssen, Ruben, Sander, Andreas A. C., Sanders, Jason L., Sargent, Mark, Sarpa, Elena, Schimd, Carlo, Schipani, Pietro, Sefusatti, Emiliano, Smith, Graham P., Spina, Lorenzo, Steinmetz, Matthias, Tacchella, Sandro, Tautvaisiene, Grazina, Theissen, Christopher, Thomas, Guillaume, Ting, Yuan-Sen, Travouillon, Tony, Tresse, Laurence, Trivedi, Oem, Tsantaki, Maria, Tsedrik, Maria, Urrutia, Tanya, Valenti, Elena, Van der Swaelmen, Mathieu, Van Eck, Sophie, Verdiani, Francesco, Verdier, Aurelien, Vergani, Susanna Diana, Verhamme, Anne, Vernet, Joel, Verza, Giovanni, Viel, Matteo, Vielzeuf, Pauline, Vietri, Giustina, Vink, Jorick S., Vazquez, Carlos Viscasillas, Wang, Hai-Feng, Weilbacher, Peter M., Wendt, Martin, Wright, Nicholas, Ye, Quanzhi, Yeche, Christophe, Yu, Jiaxi, Zafar, Tayyaba, Zibetti, Stefano, Ziegler, Bodo, Zinchenko, Igor
The Wide-field Spectroscopic Telescope (WST) is proposed as a new facility dedicated to the efficient delivery of spectroscopic surveys. This white paper summarises the initial concept as well as the corresponding science cases. WST will feature simu
Externí odkaz:
http://arxiv.org/abs/2403.05398
Autor:
Law, C-Y, Tan, Jonathan C., Skalidis, Raphael, Morgan, Larry, Xu, Duo, Alves, Felipe de Oliveira, Barnes, Ashley T., Butterfield, Natalie, Caselli, Paola, Cosentino, Giuliana, Fontani, Francesco, Henshaw, Jonathan D., Jimenez-Serra, Izaskun, Lim, Wanggi
Magnetic fields may play a crucial role in setting the initial conditions of massive star and star cluster formation. To investigate this, we report SOFIA-HAWC+ $214\:\mu$m observations of polarized thermal dust emission and high-resolution GBT-Argus
Externí odkaz:
http://arxiv.org/abs/2401.11560
Autor:
Bianchi, Eleonora, Ceccarelli, Cecilia, Codella, Claudio, López-Sepulcre, Ana, Yamamoto, Satoshi, Balucani, Nadia, Caselli, Paola, Podio, Linda, Neri, Roberto, Bachiller, Rafael, Favre, Cécile, Fontani, Francesco, Lefloch, Bertrand, Sakai, Nami, Segura-Cox, Dominique
Publikováno v:
A&A 662, A103 (2022)
We studied the line emission from CH3CN and its deuterated isotopologue CH$_2$DCN towards the prototypical Class I object SVS13-A, where the deuteration of a large number of species has already been reported. Our goal is to measure the CH$_3$CN deute
Externí odkaz:
http://arxiv.org/abs/2202.09285
Autor:
Ohashi, Satoshi, Codella, Claudio, Sakai, Nami, Chandler, Claire J., Ceccarelli, Cecilia, Alves, Felipe, Fedele, Davide, Hanawa, Tomoyuki, Durán, Aurora, Favre, Cécile, López-Sepulcre, Ana, Loinard, Laurent, Mercimek, Seyma, Murillo, Nadia M., Podio, Linda, Zhang, Yichen, Aikawa, Yuri, Balucani, Nadia, Bianchi, Eleonora, Bouvier, Mathilde, Busquet, Gemma, Caselli, Paola, Caux, Emmanuel, Charnley, Steven, Choudhury, Spandan, Cuello, Nicolas, De Simone, Marta, Dulieu, Francois, Evans, Lucy, Feng, Siyi, Fontani, Francesco, Francis, Logan, Hama, Tetsuya, Herbst, Eric, Hirano, Shingo, Hirota, Tomoya, Imai, Muneaki, Isella, Andrea, Jímenez-Serra, Izaskun, Johnstone, Doug, Kahane, Claudine, Gal, Romane Le, Lefloch, Bertrand, Maud, Luke T., Maureira, Maria Jose, Menard, Francois, Miotello, Anna, Moellenbrock, George, Mori, Shoji, Nakatani, Riouhei, Nomura, Hideko, Oba, Yasuhiro, O'Donoghue, Ross, Okoda, Yuki, Ospina-Zamudio, Juan, Oya, Yoko, Pineda, Jaime, Rimola, Albert, Sakai, Takeshi, Segura-Cox, Dominique, Shirley, Yancy, Svoboda, Brian, Taquet, Vianney, Testi, Leonardo, Vastel, Charlotte, Viti, Serena, Watanabe, Naoki, Watanabe, Yoshimasa, Witzel, Arezu, Xue, Ci, Zhao, Bo, Yamamoto, Satoshi
We report a study of the low-mass Class-0 multiple system VLA 1623AB in the Ophiuchus star-forming region, using H$^{13}$CO$^+$ ($J=3-2$), CS ($J=5-4$), and CCH ($N=3-2$) lines as part of the ALMA Large Program FAUST. The analysis of the velocity fie
Externí odkaz:
http://arxiv.org/abs/2201.07334
Autor:
De Simone, Marta, Codella, Claudio, Ceccarelli, Cecilia, López-Sepulcre, Ana, Neri, Roberto, Rivera-Ortiz, Pedro Ruben, Busquet, Gemma, Caselli, Paola, Bianchi, Eleonora, Fontani, Francesco, Lefloch, Bertrand, Oya, Yoko, Pineda, Jaime E.
There is evidence that the star formation process is linked to the intricate net of filaments in molecular clouds, which may be also due to gas compression from external triggers. We studied the southern region of the Perseus NGC 1333 molecular cloud
Externí odkaz:
http://arxiv.org/abs/2201.03434
Autor:
Entekhabi, Negar, Tan, Jonathan C., Cosentino, Giuliana, Hsu, Chia-Jung, Caselli, Paola, Walsh, Catherine, Lim, Wanggi, Henshaw, Jonathan D., Barnes, Ashley T., Fontani, Francesco, Jiménez-Serra, Izaskun
Publikováno v:
A&A 662, A39 (2022)
Infrared dark clouds (IRDCs) are cold, dense regions of the interstellar medium (ISM) that are likely to represent the initial conditions for massive star formation. It is thus important to study the physical and chemical conditions of IRDCs to provi
Externí odkaz:
http://arxiv.org/abs/2111.05379
Autor:
Evans, Lucy, Fontani, Francesco, Vastel, Charlotte, Ceccarelli, Cecilia, Caselli, Paola, López-Sepulcre, Ana, Neri, Roberto, Alves, Felipe, Chahine, Layal, Favre, Cecile, Lattanzi, Valerio
Isotopic fractionation is an important tool to investigate the chemical history of our Solar System (SS). In particular, the isotopic fraction of nitrogen (14N/15N) is lower in comets and other pristine SS bodies with respect to the value measured fo
Externí odkaz:
http://arxiv.org/abs/2110.10427
Publikováno v:
A&A 649, A149 (2021)
Recently, there has been an increased interest in the study of the generation of low-energy cosmic rays (CRs; < 1 TeV) in shocks situated on the surface of a protostar or along protostellar jets. These locally accelerated CRs offer an attractive expl
Externí odkaz:
http://arxiv.org/abs/2103.08599