Zobrazeno 1 - 10
of 33
pro vyhledávání: '"Steven R. Warren"'
Autor:
Brian Austin, Sudheer Chunduri, Nathan Wichmann, Nicholas J. Wright, Steven R. Warren, Taylor Groves, Peter Mendygral, Krishna Kandalla, Glenn K. Lockwood, Kalyan Kumaran, Scott Parker, Jacob Balma
Publikováno v:
SC
Network congestion is one of the biggest problems facing HPC systems today, affecting system throughput, performance, user experience, and reproducibility. Congestion manifests as run-to-run variability due to contention for shared resources (e.g., f
Autor:
Steven R. Warren, Margaret Meixner, Jacco Th. van Loon, J. D. Smith, Julia Roman-Duval, Remy Indebetouw, Frank P. Israel, Monica Rubio, Erik Muller, Alberto D. Bolatto, Mark G. Wolfire, Yoko Okada, Katherine Jameson, Kevin V. Croxall, Rodrigo Herrera-Camus, Eric W. Pellegrini, Celia Verdugo, Hans Zinnecker
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 853(2), 111
The Astrophysical Journal, 853(2), 111
The Small Magellanic Cloud (SMC) provides the only laboratory to study the structure of molecular gas at high resolution and low metallicity. We present results from the Herschel Spectroscopic Survey of the SMC (HS$^{3}$), which mapped the key far-IR
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28f8f2291067120bf0120b0d5f5efaab
Autor:
Alberto D. Bolatto, Laura K. Zschaechner, Nick Scoville, Rebecca C. Levy, Fabian Walter, Adam K. Leroy, Erik Rosolowsky, Martin Zwaan, Jacqueline Hodge, Sylvain Veilleux, David S. Meier, Jürgen Ott, Eve C. Ostriker, Steven R. Warren, Axel Weiss
Publikováno v:
ASTROPHYSICAL JOURNAL (ISSN 0004-637X), 835, 265
We present a detailed study of a molecular outflow feature in the nearby starburst galaxy NGC 253 using ALMA. We find that this feature is clearly associated with the edge of NGC 253's prominent ionized outflow, has a projected length of ~300 pc, wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::245ea44d58e76eb7c8ad4f9e9adde97a
https://doi.org/10.3847/1538-4357/835/2/265
https://doi.org/10.3847/1538-4357/835/2/265
Autor:
Edward C. Elson, Andrew McNichols, Amelie Saintonge, Elizabeth A. K. Adams, Angela Van Sistine, Steven R. Warren, Ian Cave, Jürgen Ott, Melissa V. Marshall, Elise Nims, Clara M. Thomann, Gyula I. G. Józsa, Riccardo Giovanelli, Andrew E. Dolphin, Shan Huang, Nathalie C. Haurberg, Elijah Z. Bernstein-Cooper, Evan D. Skillman, John M. Cannon, Steven Janowiecki, Yaron Teich, John J. Salzer, Cedric Hagen, Kristen B. W. McQuinn, Martha P. Haynes
We analyze the relationships between atomic, neutral hydrogen (HI) and star formation (SF) in the 12 low-mass SHIELD galaxies. We compare high spectral (~0.82 km/s/channel) and spatial resolution (physical resolutions of 170 pc - 700 pc) HI imaging f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0107602b41c269f3ba11a2ea216fe39a
Autor:
Alberto D. Bolatto, N. M. Förster Schreiber, Linda J. Tacconi, Andreas Burkert, David Fisher, Steven R. Warren, Amélie Saintonge, Stijn Wuyts, Achim Weiss, Reinhard Genzel, F. Bournaud, Francoise Combes, Adam Leroy, Santiago García-Burillo, M. C. Cooper, Nicolas Bouché, Amiel Sternberg
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2015, 809 (2), pp.175. ⟨10.1088/0004-637X/809/2/175⟩
The Astrophysical Journal, 2015, 809 (2), pp.175. ⟨10.1088/0004-637X/809/2/175⟩
The Astrophysical Journal, American Astronomical Society, 2015, 809 (2), pp.175. ⟨10.1088/0004-637X/809/2/175⟩
The Astrophysical Journal, 2015, 809 (2), pp.175. ⟨10.1088/0004-637X/809/2/175⟩
We present Karl G. Jansky Very Large Array observations of the CO J=1-0 transition in a sample of four $z\sim2$ main sequence galaxies. These galaxies are in the blue sequence of star-forming galaxies at their redshift, and are part of the IRAM Plate
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bbf679a7bf92a80c1ccac741cf180516
https://hal.archives-ouvertes.fr/hal-02395810
https://hal.archives-ouvertes.fr/hal-02395810
Publikováno v:
Publications of the Astronomical Society of the Pacific. 118:1373-1389
Multicolor (BVRI) light curves of the eclipsing novalike variable TT Tri are presented and analyzed with a parameter-fitting eclipse model. The mass ratio of TT Tri is poorly constrained, but must lie roughly in the range 0.3>R_1) generally resulted
Publikováno v:
International Oil Spill Conference Proceedings. 2003:477-482
In the late 1980s, the United Nations recognized that industrial activities of the 19th and 2(20th centuries were responsible for global pollution-related problems, and presented a future threat to life-sustaining qualities of the environment. While
Autor:
Evan D. Skillman, Edward C. Elson, John M. Cannon, Katherine L. Rhode, Steven R. Warren, Elizabeth A. K. Adams, Jayaram Chengular, John J. Salzer, Martha P. Haynes, Alberto D. Bolatto, Kristen B. W. McQuinn, Riccardo Giovanelli, Stephen A. Pardy, Elijah Z. Bernstein-Cooper
We present new HI spectral line imaging of the extremely metal-poor, star-forming dwarf irregular galaxy Leo P. Our HI images probe the global neutral gas properties and the local conditions of the interstellar medium (ISM). The HI morphology is slig
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77e9737c14c704e46c19e2fee653b742
http://arxiv.org/abs/1404.5298
http://arxiv.org/abs/1404.5298
Autor:
Fabian Walter, Alberto D. Bolatto, Martin Zwaan, Sylvain Veilleux, Andreas Schruba, Eve C. Ostriker, Karin Sandstrom, Adam K. Leroy, David S. Meier, Erik Rosolowsky, Steven R. Warren, Jennifer Donovan Meyer, Jacqueline Hodge, Jürgen Ott
We use ALMA to derive the mass, length, and time scales associated with the nuclear starburst in NGC 253. This region forms ~2 M_sun/yr of stars and resembles other starbursts in scaling relations, with star formation consuming the gas reservoir 10 t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::08b75b9b7193709ea7a293c8c3fcf96e
Autor:
Steven R. Warren, Evan D. Skillman, Juergen Ott, Julianne J. Dalcanton, Baerbel Koribalski, Adrienne M. Stilp
Neutral hydrogen (HI) velocity dispersions are believed to be set by turbulence in the interstellar medium (ISM). Although turbulence is widely believed to be driven by star formation (SF), recent studies have shown that this driving mechanism may no
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e9bc4b05f846df80e8b7f0fc1418c584
http://arxiv.org/abs/1306.2321
http://arxiv.org/abs/1306.2321