Zobrazeno 1 - 10
of 143
pro vyhledávání: '"J.-D T. Smith"'
Autor:
Elizabeth Tarantino, Alberto D. Bolatto, Rémy Indebetouw, Mónica Rubio, Karin M. Sandstrom, J.-D T. Smith, Daniel Stapleton, Mark Wolfire
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 2, p 101 (2024)
We present Cloudy modeling of infrared emission lines in the Wolf–Rayet (WR) nebula N76 caused by one of the most luminous and hottest WR stars in the low metallicity Small Magellanic Cloud. We use spatially resolved mid-infrared Spitzer/InfRared S
Externí odkaz:
https://doaj.org/article/0efe6321f1c34c2c8303db54a13c737f
Publikováno v:
The Astrophysical Journal. 948:88
With the start of JWST observations, mid-infrared (MIR) emission features from polycyclic aromatic hydrocarbons (PAHs), H$_2$ rotational lines, fine-structure lines from ions, and dust continuum will be widely available tracers of gas and star format
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cbafe35e733501197b7df392cd6a172a
https://doi.org/10.3847/1538-4357/acc316
https://doi.org/10.3847/1538-4357/acc316
Autor:
Thomas S.-Y. Lai, Lee Armus, Vivian U, Tanio Díaz-Santos, Kirsten L. Larson, Aaron Evans, Matthew A. Malkan, Philip Appleton, Jeff Rich, Francisco Müller-Sánchez, Hanae Inami, Thomas Bohn, Jed McKinney, Luke Finnerty, David R. Law, Sean T. Linden, Anne M. Medling, George C. Privon, Yiqing Song, Sabrina Stierwalt, Paul P. van der Werf, Loreto Barcos-Muñoz, J. D. T. Smith, Aditya Togi, Susanne Aalto, Torsten Böker, Vassilis Charmandaris, Justin Howell, Kazushi Iwasawa, Francisca Kemper, Joseph M. Mazzarella, Eric J. Murphy, Michael J. I. Brown, Christopher C. Hayward, Jason Marshall, David Sanders, Jason Surace
Publikováno v:
Astrophysical Journal Letters, 941(2), L36
We present James Webb Space Telescope (JWST) Mid-Infrared Instrument (MIRI) integral-field spectroscopy of the nearby merging, luminous infrared galaxy, NGC 7469. This galaxy hosts a Seyfert type-1.5 nucleus, a highly ionized outflow, and a bright, c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d09464ae3bfdaa4b4a9a6f9188fc676
https://hdl.handle.net/1887/3561913
https://hdl.handle.net/1887/3561913
Autor:
Andrew I. Harris, Kevin V. Croxall, Mark G. Wolfire, Denise Riquelme, Christof Buchbender, Alberto D. Bolatto, Rodrigo Herrera-Camus, J. D. T. Smith, Daniel A. Dale, Jürgen Stutzki, Elizabeth Tarantino, Brent Groves, Rebecca C. Levy
The [CII] fine-structure transition at 158 micron is frequently the brightest far-infrared line in galaxies. Due to its low ionization potential, C+ can trace the ionized, atomic, and molecular phases of the ISM. We present velocity resolved [CII] an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::978d8f253fa6b2a0d4a702d3d2ee27cd
http://arxiv.org/abs/2104.13452
http://arxiv.org/abs/2104.13452
Autor:
Alberto D. Bolatto, Eric W. Pelligrini, Jessica Sutter, George Helou, Maud Galametz, Leslie K. Hunt, Kevin V. Croxall, Karin Sandstrom, Brent Groves, J. D. T. Smith, Daniel A. Dale, Christine D. Wilson, Rodrigo Herrera-Camus, Robert C. Kennicutt, Mark G. Wolfire, Médéric Boquien, Ilse De Looze, Daniela Calzetti
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
The [CII] deficit, which describes the observed decrease in the ratio of [CII] 158 micron emission to continuum infrared emission in galaxies with high star formation surface densities, places a significant challenge to the interpretation of [CII] de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e682c1f0d90c250a8314d7dc89f033b
http://arxiv.org/abs/2102.08865
http://arxiv.org/abs/2102.08865
Autor:
Daniel A. Dale, G. Aniano, Karl D. Gordon, Adam K. Leroy, Fabian Walter, J. D. T. Smith, A. D. Bolatto, J. Hinz, Robert C. Kennicutt, L. K. Hunt, Monica Relaño, Bruce T. Draine, M. Galametz, Marc Sauvage, M. Boquien, Mark Wolfire, C. W. Engelbracht, Eric J. Murphy, Eva Schinnerer, E. Montiel, Jun Koda, D. Calzetti, L. Armus, Karin Sandstrom, H. Roussel, A. Crocker, R. Skibba, I. De Looze, George Helou, J. DDonovan Meyer, B. D. Johnson, Adam Miller, H. W. Rix
ERRATUM.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a756b9e386870f8a22bb12728254fab2
http://hdl.handle.net/20.500.12386/31097
http://hdl.handle.net/20.500.12386/31097
We present a large sample of 2.5-38 $\mu m$ galaxy spectra drawn from a cross-archival comparison in the AKARI-Spitzer Extragalactic Spectral Survey (ASESS), and investigate a subset of 113 star-forming galaxies with prominent polycyclic aromatic hyd
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af8295a2424a10189a29c9502f62c4be
Publikováno v:
The Astrophysical Journal. 917:3
Using physical models, we study the sensitivity of polycyclic aromatic hydrocarbon (PAH) emission spectra to the character of the illuminating starlight, to the PAH size distribution, and to the PAH charge distribution. Starlight models considered ra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c62921dab579185639c3441e6f134084
https://doi.org/10.3847/1538-4357/abff51
https://doi.org/10.3847/1538-4357/abff51
Autor:
Mark Wolfire, J. D. T. Smith, Elias Brinks, Eric J. Murphy, Eric W. Pellegrini, Lee Armus, Eva Schinnerer, Leslie K. Hunt, Daniel A. Dale, Bruce T. Draine, Christine D. Wilson, Rodrigo Herrera-Camus, Karin Sandstrom, Alison F. Crocker, Robert C. Kennicutt, Dimitra Rigopoulou, Brent Groves, Erik Rosolowsky, Paul van der Werf
Publikováno v:
University of Hertfordshire
Astrophysical Journal (0004-637X), 887(1), 105
Astrophysical Journal (0004-637X), 887(1), 105
We present resolved [CI] line intensities of 18 nearby galaxies observed with the SPIRE FTS spectrometer on the Herschel Space Observatory. We use these data along with resolved CO line intensities from $J_\mathrm{up} = 1$ to 7 to interpret what phas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::37b4f56420a93a2d5de1c898ab045a8f
https://doi.org/10.3847/1538-4357/ab4196
https://doi.org/10.3847/1538-4357/ab4196