Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Shaye Storm"'
We use NH3 inversion transitions to trace the dense gas in the NGC 1333 region of the Perseus molecular cloud. NH3(1,1) and NH3(2,2) maps covering an area of 102 square arcminutes at an angular resolution of ~3.7" are produced by combining VLA interf
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2906559e407765f7192ca36cb5e3b16d
We present H13CO+ (J=1-0) and HNC (J=1-0) maps of regions in Serpens South, Serpens Main and NGC 1333 containing filaments. We also observe the Serpens regions using H13CN (J=1-0). These dense gas tracer molecular line observations carried out with C
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::419370f7f64d7e77809f7dbf621891c2
http://arxiv.org/abs/1801.03155
http://arxiv.org/abs/1801.03155
Autor:
C. Waelkens, Shaye Storm, Nuria Calvet, Leonardo Testi, Joseph Lazio, Jane Greaves, David J. Wilner, Woojin Kwon, Laura M. Pérez, Cornelis P. Dullemond, Sean M. Andrews, Stuartt Corder, Claire J. Chandler, Lee G. Mundy, H. Linz, A. I. Sargent, Myriam Benisty, Adam Deller, Th. Henning, Luca Ricci, R. van Boekel, Robert J. Harris, J. Menu, Andrea Isella, John M. Carpenter
Publikováno v:
Proceedings of the International Astronomical Union. 8:104-108
For over a decade, the structure of the inner “hole” in the transition disk around TW Hydrae has been a subject of debate. To probe the innermost regions of the protoplanetary disk, observations at the highest possible spatial resolution are requ
Autor:
Hector G. Arce, Erin G. Cox, Shaye Storm, Robert J. Harris, Leslie W. Looney, Peter Teuben, M. Fernández-López, Lee G. Mundy
Publikováno v:
Proceedings of the 71st International Symposium on Molecular Spectroscopy.
Autor:
Marc W. Pound, John J. Tobin, Konstantinos Tassis, Erik Rosolowsky, Aaron M. Meisner, Adele Plunkett, Dominique Segura-Cox, Shaye Storm, Richard M. Crutcher, Katherine I. Lee, Manuel Fernández-López, Leonardo Testi, Yancy L. Shirley, Jens Kauffmann, Lee G. Mundy, Nikolaus H. Volgenau, Leslie W. Looney, Héctor G. Arce, Andrea Isella, Woojin Kwon, Peter Teuben
Publikováno v:
ASTROPHYSICAL JOURNAL
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
ASTROPHYSICAL JOURNAL, 830(2), 127
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
ASTROPHYSICAL JOURNAL, 830(2), 127
We present a 3 mm spectral line and continuum survey of L1451 in the Perseus Molecular Cloud. These observations are from the CARMA Large Area Star Formation Survey (CLASSy), which also imaged Barnard 1, NGC 1333, Serpens Main and Serpens South. L145
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e0e097d69b6dd23116a20c41a8a5226
https://hdl.handle.net/1887/47814
https://hdl.handle.net/1887/47814
Autor:
Joseph Lazio, Laura M. Pérez, Th. Henning, Stuartt Corder, David J. Wilner, Sergio Ortolani, Sean M. Andrews, Andrea Isella, John M. Carpenter, Leonardo Testi, Marco Tazzari, Shaye Storm, Lee G. Mundy, Nuria Calvet, Jane Greaves, H. Linz, I. de Gregorio-Monsalvo, Adam Deller, A. Natta, Luca Ricci, Woojin Kwon, Claire J. Chandler, G Guidi, A. I. Sargent, Cornelis P. Dullemond
Publikováno v:
NASA Astrophysics Data System
To characterize the mechanisms of planet formation it is crucial to investigate the properties and evolution of protoplanetary disks around young stars, where the initial conditions for the growth of planets are set. Our goal is to study grain growth
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9055a59602665b35fee3ad334a39e54a
http://hdl.handle.net/11577/3230325
http://hdl.handle.net/11577/3230325
Autor:
Luca Ricci, Nuria Calvet, A. Natta, Sean M. Andrews, Andrea Isella, Marco Tazzari, Lee G. Mundy, John M. Carpenter, H. Linz, Adam Deller, Leonardo Testi, Shaye Storm, David J. Wilner, Joseph Lazio, Woojin Kwon, Laura M. Pérez, Barbara Ercolano, Stuartt Corder, J. A. Greaves, Th. Henning, Claire J. Chandler, Cornelis P. Dullemond, A. I. Sargent
Publikováno v:
NASA Astrophysics Data System
Theoretical models of grain growth predict dust properties to change as a function of protoplanetary disk radius, mass, age and other physical conditions. We lay down the methodology for a multi-wavelength analysis of (sub-)mm and cm continuum interf
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cce67b8ce5dd1569cde75dbea880abb8
http://arxiv.org/abs/1512.05679
http://arxiv.org/abs/1512.05679
Autor:
Woojin Kwon, Jane S. Greaves, Thomas Henning, John M. Carpenter, Claire J. Chandler, Lee G. Mundy, Shaye Storm, Andrea Isella, Adam Deller, Nuria Calvet, Sean M. Andrews, Joseph Lazio, Marco Tazzari, Stuartt Corder, Hendrik Linz, Leonardo Testi, Luca Ricci, Laura M. Pérez, Anneila I. Sargent, Robert J. Harris, Cornelis P. Dullemond, David J. Wilner
We present new results from the Disks@EVLA program for two young stars: CY Tau and DoAr 25. We trace continuum emission arising from their circusmtellar disks from spatially resolved observations, down to tens of AU scales, at {\lambda} = 0.9, 2.8, 8
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f7dc901771f755a81d46ea45615be37b
https://resolver.caltech.edu/CaltechAUTHORS:20200131-132810636
https://resolver.caltech.edu/CaltechAUTHORS:20200131-132810636
Autor:
Maxime Rizzo, Manuel Fernández-López, Robert J. Harris, Shaye Storm, Héctor G. Arce, Dominique Segura-Cox, Lee G. Mundy, Katherine I. Lee, Leslie W. Looney
Publikováno v:
Proceedings of the 70th International Symposium on Molecular Spectroscopy.
Autor:
Konrad Smiarowski, Yekaterina Krivogorskaya, Malgorzata Frik, Shaye Storm, Colin Amundsen, Monica Koczela, Salena Modugno, Thomas H. McGovern, Matthew Matthew Brown, Sophia Perdikaris
Publikováno v:
Environmental Archaeology. 10:127-142
Excavations in 1990 in North-West Iceland documented a stratified series of small turf structures and associated midden deposits at the eroding beach at Akurvik which date from the 11th–13th to the 15th–16th centuries AD. The site reflects a long