Zobrazeno 1 - 10
of 130
pro vyhledávání: '"Evans, Lucy P."'
Autor:
Temmink, Milou, Booth, Alice S., Leemker, Margot, van der Marel, Nienke, van Dishoeck, Ewine F., Evans, Lucy, Keyte, Luke, Law, Charles J., Notsu, Shota, Öberg, Karin, Walsh, Catherine
The ongoing physical and chemical processes in planet-forming disks set the stage for planet formation. The asymmetric disk around the young star Oph-IRS 48 has one of the most well-characterised chemical inventories, showing molecular emission from
Externí odkaz:
http://arxiv.org/abs/2411.12418
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:
Booth, Alice S., Leemker, Margot, van Dishoeck, Ewine F., Evans, Lucy, Ilee, John D., Kama, Mihkel, Keyte, Luke, Law, Charles J., van der Marel, Nienke, Nomura, Hideko, Notsu, Shota, Öberg, Karin, Temmink, Milou, Walsh, Catherine
Observations of disks with the Atacama Large Millimeter/submillimeter Array (ALMA) allow us to map the chemical makeup of nearby protoplanetary disks with unprecedented spatial resolution and sensitivity. The typical outer Class II disk observed with
Externí odkaz:
http://arxiv.org/abs/2402.04001
Autor:
Booth, Alice S., Temmink, Milou, van Dishoeck, Ewine F., Evans, Lucy, Ilee, John D., Kama, Mihkel, Keyte, Luke, Law, Charles J., Leemker, Margot, van der Marel, Nienke, Nomura, Hideko, Notsu, Shota, Öberg, Karin, Walsh, Catherine
The Atacama Large Millimeter/submillimeter Array (ALMA) can probe the molecular content of planet-forming disks with unprecedented sensitivity. These observations allow us to build up an inventory of the volatiles available for forming planets and co
Externí odkaz:
http://arxiv.org/abs/2402.04002
Autor:
Evans, Lucy, Vastel, Charlotte, Fontani, Francisco, Pineda, Jaime, Jiménez-Serra, Izaskun, Alves, Felipe, Sakai, Takeshi, Bouvier, Mathilde, Caselli, Paola, Ceccarelli, Cecilia, Chandler, Claire, Svoboda, Brian, Maud, Luke, Codella, Claudio, Sakai, Nami, Gal, Romane Le, López-Sepulcre, Ana, Moellenbrock, George, Yamamoto, Satoshi
Publikováno v:
A&A 678, A160 (2023)
Context. Deuterium in H-bearing species is enhanced during the early stages of star formation, however, only a small number of high spatial resolution deuteration studies exist towards protostellar objects, leaving the small-scale structures unreveal
Externí odkaz:
http://arxiv.org/abs/2309.00501
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:
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
Autor:
Okoda, Yuki, Oya, Yoko, Francis, Logan, Johnstone, Doug, Inutsuka, Shu-ichiro, Ceccarelli, Cecilia, Codella, Claudio, Chandler, Claire, Sakai, Nami, Aikawa, Yuri, Alves, Felipe, Balucani, Nadia, Bianchi, Eleonora, Bouvier, Mathilde, Caselli, Paola, Caux, Emmanuel, Charnley, Steven, Choudhury, Spandan, De Simone, Marta, Dulieu, Francois, Durán, Aurora, Evans, Lucy, Favre, Cécile, Fedele, Davide, Feng, Siyi, Fontani, Francesco, Hama, Tetsuya, Hanawa, Tomoyuki, Herbst, Eric, Hirota, Tomoya, Imai, Muneaki, Isella, Andrea, Jímenez-Serra, Izaskun, Kahane, Claudine, Lefloch, Bertrand, Loinard, Laurent, López-Sepulcre, Ana, Maud, Luke T., Maureira, Maria Jose, Menard, Francois, Mercimek, Seyma, Miotello, Anna, Moellenbrock, George, Mori, Shoji, Murillo, Nadia M., Nakatani, Riouhei, Nomura, Hideko, Oba, Yasuhiro, O'Donoghue, Ross, Ohashi, Satoshi, Ospina-Zamudio, Juan, Pineda, Jaime, Podio, Linda, Rimola, Albert, Sakai, Takeshi, Cox, Dominique Segura, Shirley, Yancy, Svoboda, Brian, Taquet, Vianney, Testi, Leonardo, Vastel, Charlotte, Viti, Serena, Watanabe, Naoki, Watanabe, Yoshimasa, Witzel, Arezu, Xue, Ci, Zhang, Yichen, Zhao, Bo, Yamamoto, Satoshi
We have observed the very low-mass Class 0 protostar IRAS 15398-3359 at scales ranging from 50 au to 1800 au, as part of the ALMA Large Program FAUST. We uncover a linear feature, visible in H2CO, SO, and C18O line emission, which extends from the so
Externí odkaz:
http://arxiv.org/abs/2101.07404
Akademický článek
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Autor:
Harper, Matthew M., Rudd, Danielle, Meyer, Kacie J., Kanthasamy, Anumantha. G., Anantharam, Vellareddy, Pieper, Andrew A., Vázquez-Rosa, Edwin, Shin, Min-Kyoo, Chaubey, Kalyani, Koh, Yeojung, Evans, Lucy P., Bassuk, Alexander G., Anderson, Michael G., Dutca, Laura, Kudva, Indira T., John, Manohar
Publikováno v:
In Heliyon February 2020 6(2)
