Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Walmsley, C. Malcolm"'
Autor:
Wang, Ke, Testi, Leonardo, Burkert, Andreas, Walmsley, C. Malcolm, Beuther, Henrik, Henning, Thomas
Large-scale gaseous filaments with length up to the order of 100 pc are on the upper end of the filamentary hierarchy of the Galactic interstellar medium. Their association with respect to the Galactic structure and their role in Galactic star format
Externí odkaz:
http://arxiv.org/abs/1607.06452
Autor:
Wang, Ke, Testi, Leonardo, Ginsburg, Adam, Walmsley, C. Malcolm, Molinari, Sergio, Schisano, Eugenio
Publikováno v:
MNRAS 2015, Volume 450, p.4043-4049
The ubiquity of filamentary structure at various scales through out the Galaxy has triggered a renewed interest in their formation, evolution, and role in star formation. The largest filaments can reach up to Galactic scale as part of the spiral arm
Externí odkaz:
http://arxiv.org/abs/1504.00647
Autor:
Merello, Manuel, Bronfman, Leonardo, Garay, Guido, Nyman, Lars-Ake, Evans II, Neal J., Walmsley, C. Malcolm
We report molecular line and dust continuum observations toward the high-mass star forming region G331.5-0.1, one of the most luminous regions of massive star-formation in the Milky Way, located at the tangent region of the Norma spiral arm, at a dis
Externí odkaz:
http://arxiv.org/abs/1306.0042
Autor:
Caselli, Paola, Keto, Eric, Bergin, Edwin A., Tafalla, Mario, Aikawa, Yuri, Douglas, Thomas, Pagani, Laurent, Yildiz, Umut A., van der Tak, Floris F. S., Walmsley, C. Malcolm, Codella, Claudio, Nisini, Brunella, Kristensen, Lars E., van Dishoeck, Ewine F.
Water is a crucial molecule in molecular astrophysics as it controls much of the gas/grain chemistry, including the formation and evolution of more complex organic molecules in ices. Pre-stellar cores provide the original reservoir of material from w
Externí odkaz:
http://arxiv.org/abs/1208.5998
We used the IRAM Interferometer to obtain sub-arcsecond resolution observations of the high-mass star-forming region W3(OH) and its surroundings at a frequency of 220 GHz. With the improved angular resolution, we distinguish 3 peaks in the thermal du
Externí odkaz:
http://arxiv.org/abs/astro-ph/9901261
Autor:
Ke Wang, Testi, Leonardo, Ginsburg, Adam, Walmsley, C. Malcolm, Molinari, Sergio, Schisano, Eugenio
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 7/11/2015, Vol. 450 Issue 4, p4043-4049, 7p
Autor:
Sanchez-Monge, Alvaro, Cesaroni, Riccardo, Beltran, Maite, Kumar, M. S. Nanda, Stanke, Thomas, Zinnecker, Hans, Etoka, Sandra, Galli, Daniele, Hummel, Christian A., Luca Moscadelli, Preibisch, Thomas, Ratzka, Thorsten, Tak, Floris F. S., Vig, Sarita, Walmsley, C. Malcolm, Wang, Kuo-Song
Publikováno v:
NASA Astrophysics Data System
Protostars and Planets VI
Protostars and Planets VI
Recent theoretical models indicate that OB-type stars could form through disk-mediated accretion, like their low mass counterparts. However, on the observational side, circumstellar disks appear still elusive, especially around the most massive (prot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::4af39684e02dec9572e93117dc43ef42
https://ui.adsabs.harvard.edu/#abs/2013prpl.conf1B045S
https://ui.adsabs.harvard.edu/#abs/2013prpl.conf1B045S