Zobrazeno 1 - 10
of 128
pro vyhledávání: '"Woods, Paul M"'
Autor:
Gokus, Andrea, Jahnke, Knud, Woods, Paul M, Moss, Vanessa A, Ossenkopf-Okada, Volker, Sacchi, Elena, Stevens, Adam R H, Burtscher, Leonard, Kayhan, Cenk, Dalgleish, Hannah, Grinberg, Victoria, Rector, Travis A, Rybizki, Jan, White, Jacob
Publikováno v:
PNAS Nexus, Volume 3, Issue 5, May 2024, pgae143
Travel to academic conferences -- where international flights are the norm -- is responsible for a sizeable fraction of the greenhouse gas (GHG) emissions associated with academic work. In order to provide a benchmark for comparison with other fields
Externí odkaz:
http://arxiv.org/abs/2405.00104
Autor:
Jones, Olivia C., Woods, Paul M., Kemper, F., Kraemer, K. E., Sloan, G. C., Srinivasan, S., Oliveira, J. M., van Loon, J. Th., Boyer, Martha L., Sargent, Benjamin A., McDonald, I., Meixner, Margaret, Zijlstra, A. A., Ruffle, Paul M. E., Lagadec, E., Pauly, Tyler, Sewiło, Marta, Clayton, G. C., Volk, K.
The Infrared Spectrograph (IRS) on the {\em Spitzer Space Telescope} observed nearly 800 point sources in the Large Magellanic Cloud (LMC), taking over 1,000 spectra. 197 of these targets were observed as part of the Sage-Spec Spitzer Legacy program;
Externí odkaz:
http://arxiv.org/abs/1705.02709
Autor:
Matsuura, Mikako, Sargent, B., Swinyard, Bruce, Yates, Jeremy, Royer, P., Barlow, M. J., Boyer, Martha, Decin, L., Khouri, Theo, Meixner, Margaret, van Loon, Jacco Th., Woods, Paul M.
Using the PACS and SPIRE spectrometers on-board the Herschel Space Observatory, we obtained spectra of two red supergiants (RSGs) in the Large Magellanic Cloud (LMC). Multiple rotational CO emission lines (J=6-5 to 15-14) and 15 H2O lines were detect
Externí odkaz:
http://arxiv.org/abs/1608.01729
Autor:
Ruffle, Paul M. E., Kemper, F., Jones, O. C., Sloan, G. C., Kraemer, K. E., Woods, Paul M., Boyer, M. L., Srinivasan, S., Antoniou, V., Lagadec, E., Matsuura, M., McDonald, I., Oliveira, J. M., Sargent, B. A., Sewilo, M., Szczerba, R., van Loon, J. Th., Volk, K., Zijlstra, A. A.
The Magellanic clouds are uniquely placed to study the stellar contribution to dust emission. Individual stars can be resolved in these systems even in the mid-infrared, and they are close enough to allow detection of infrared excess caused by dust.W
Externí odkaz:
http://arxiv.org/abs/1505.04499
Autor:
Woods, Paul M., Occhiogrosso, Angela, Viti, Serena, Kanuchova, Z., Palumbo, Maria Elisabetta, Price, Stephen D.
Sulfur appears to be depleted by an order of magnitude or more from its elemental abundance in star-forming regions. In the last few years, numerous observations and experiments have been performed in order to to understand the reasons behind this de
Externí odkaz:
http://arxiv.org/abs/1503.07227
Autor:
Sargent, Benjamin A., Srinivasan, S., Meixner, M., Kemper, F., Tielens, A. G. G. M., Speck, A. K., Matsuura, M., Bernard, J. -Ph., Hony, S., Gordon, Karl D., Indebetouw, R., Marengo, M., Sloan, G. C., Woods, Paul M.
Publikováno v:
vol. 716, 2010, pp. 878-890
We model multi-wavelength broadband UBVIJHKs and Spitzer IRAC and MIPS photometry and IRS spectra from the SAGE and SAGE-Spec observing programs of two oxygen-rich asymptotic giant branch (O-rich AGB) stars in the Large Magellanic Cloud (LMC) using r
Externí odkaz:
http://arxiv.org/abs/1407.6996
Autor:
Calcutt, Hannah, Viti, Serena, Codella, Claudio, Beltrán, Maria T., Fontani, Francesco, Woods, Paul M.
We present the results of a line identification analysis using data from the IRAM Plateau de Bure Inferferometer, focusing on six massive star-forming hot cores: G31.41+0.31, G29.96-0.02, G19.61-0.23, G10.62-0.38, G24.78+0.08A1 and G24.78+0.08A2. We
Externí odkaz:
http://arxiv.org/abs/1407.1661
Autor:
Matsuura, Mikako, Bernard-Salas, Jeronimo, Evans, T. Lloyd, Volk, Kevin M., Hrivnak, Bruce J., Sloan, G. C., Chu, You-Hua, Gruendl, Robert, Kraemer, Kathleen E., Peeters, Els, Szczerba, R., Wood, P. R., Zijlstra, Albert A., Hony, S., Ita, Yoshifusa, Kamath, Devika, Lagadec, Eric, Parker, Quentin A, Reid, Warren A., Shimonishi, Takashi, Van Winckel, H., Woods, Paul M., Kemper, F., Meixner, Margaret, Otsuka, M., Sahai, R., Sargent, B. A., Hora, J. L., McDonald, Iain
This paper reports variations of polycyclic aromatic hydrocarbons (PAHs) features that were found in Spitzer Space Telescope spectra of carbon-rich post-asymptotic giant branch (post-AGB) stars in the Large Magellanic Cloud (LMC). The paper consists
Externí odkaz:
http://arxiv.org/abs/1401.0728
Glycolaldehyde, the simplest monosaccharide sugar, has recently been detected in low- and high-mass star-forming cores. Following on from our previous investigation into glycolaldehyde formation (Woods et al. 2012, ApJ, 750, 19), we now consider a fu
Externí odkaz:
http://arxiv.org/abs/1309.1164
In order to understand the evolution of the interstellar medium (ISM) of a galaxy, we have analysed the gas and dust budget of the Small Magellanic Cloud (SMC). Using the Spitzer Space Telescope, we measured the integrated gas mass-loss rate across a
Externí odkaz:
http://arxiv.org/abs/1212.1468