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pro vyhledávání: '"Hogge, Taylor"'
Autor:
Hogge, Taylor Graham
Since high-mass stars form deeply embedded within dense molecular clumps, the evolution of young stars and of dense clumps is inextricably linked. Previous datasets, however, lack the information necessary to test the prevailing theories. Definitive
Externí odkaz:
https://hdl.handle.net/2144/44800
Autor:
Stephens, Ian W., Myers, Philip C., Zucker, Catherine, Jackson, James M., Andersson, B-G, Smith, Rowan, Soam, Archana, Battersby, Cara, Sanhueza, Patricio, Hogge, Taylor, Smith, Howard A., Novak, Giles, Sadavoy, Sarah, Pillai, Thushara, Li, Zhi-Yun, Looney, Leslie W., Sugitani, Koji, Coude, Simon, Guzman, Andres, Goodman, Alyssa, Kusune, Takayoshi, Santos, Fabio P., Zuckerman, Leah, Encalada, Frankie
Star formation primarily occurs in filaments where magnetic fields are expected to be dynamically important. The largest and densest filaments trace spiral structure within galaxies. Over a dozen of these dense ($\sim$10$^4$\,cm$^{-3}$) and long ($>$
Externí odkaz:
http://arxiv.org/abs/2201.11933
Autor:
Jackson, James M., Allingham, David, Killerby-Smith, Nicholas, Whitaker, J. Scott, Smith, Howard A., Contreras, Yanett, Guzman, Andres E., Hogge, Taylor, Sanhueza, Patricio, Stephens, Ian W.
Because the 157.74 micron [C II] line is the dominant coolant of star-forming regions, it is often used to infer the global star-formation rates of galaxies. By characterizing the [C II] and far-infrared emission from nearby Galactic star-forming mol
Externí odkaz:
http://arxiv.org/abs/2009.09098
Akademický článek
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Autor:
Hogge, Taylor G., Jackson, James M., Allingham, David, Guzman, Andres E., Killerby-Smith, Nicholas, Kraemer, Kathleen E., Sanhueza, Patricio, Stephens, Ian W., Whitaker, J. Scott
G23.33-0.30 is a 600 $M_{\odot}$ infrared dark molecular filament that exhibits large NH$_3$ velocity dispersions ($\sigma \sim 8 \ \rm{km \ s^{-1}}$) and bright, narrow NH$_3$(3,3) line emission. We have probed G23.33-0.30 at the $<0.1$ pc scale and
Externí odkaz:
http://arxiv.org/abs/1910.13070
Autor:
Hogge, Taylor, Jackson, James, Stephens, Ian, Whitaker, Scott, Foster, Jonathan, Camarata, Matthew, Roshi, D. Anish, Di Francesco, James, Longmore, Steven, Loughnane, Robert, Moore, Toby, Rathborne, Jill, Sanhueza, Patricio, Walsh, Andrew
Publikováno v:
Hogge, T. G., Jackson, J. M., Stephens, I. W. et al. 2018, ApJS, 237, 27
The Radio Ammonia Mid-Plane Survey (RAMPS) is a molecular line survey that aims to map a portion of the Galactic midplane in the first quadrant of the Galaxy (l = 10 deg - 40 deg, |b| < 0.4 deg) using the Green Bank Telescope. We present results from
Externí odkaz:
http://arxiv.org/abs/1808.02533