Zobrazeno 1 - 10
of 10
pro vyhledávání: '"J. L. Hinz"'
Autor:
I. De Looze, Stefano Zibetti, Laura Silva, L. K. Hunt, Andrea Rossi, Karl D. Gordon, Bruce T. Draine, Jin Koda, D. Calzetti, K. V. Croxall, Bernhard R. Brandl, Karin Sandstrom, Robert C. Kennicutt, M. Galametz, Jd Smith, George Helou, Samir Salim, M. Boquien, Daniel A. Dale, Monica Relaño, Christine D. Wilson, Stefano Bianchi, Gian Luigi Granato, L. Ciesla, J. L. Hinz, Rodrigo Herrera-Camus, R. Nikutta, S. Viaene, Brent Groves
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 621, pp.A51. ⟨10.1051/0004-6361/201834212⟩
Astronomy and Astrophysics (0004-6361), 621, A51
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A, 2019, 621, pp.A51. ⟨10.1051/0004-6361/201834212⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 621, pp.A51. ⟨10.1051/0004-6361/201834212⟩
Astronomy and Astrophysics (0004-6361), 621, A51
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A, 2019, 621, pp.A51. ⟨10.1051/0004-6361/201834212⟩
We have fit the far-ultraviolet (FUV) to sub-millimeter (850 micron) spectral energy distributions (SEDs) of the 61 galaxies from the "Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel" (KINGFISH). The fitting has been performed us
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c959e920ff31f8a4f0492b49ffe563a2
https://hal.archives-ouvertes.fr/hal-03376259
https://hal.archives-ouvertes.fr/hal-03376259
Autor:
J. D. T. Smith, Bruce T. Draine, Karl D. Gordon, Leslie K. Hunt, Charles W. Engelbracht, Brent Groves, Marc Sauvage, Benjamin D. Johnson, Lee Armus, George Helou, Jin Koda, Bernhard R. Brandl, Kevin V. Croxall, Stefano Zibetti, Yongbao Li, P. Beirao, P. N. Appleton, Maud Galametz, Karin Sandstrom, Helene Roussel, J. L. Hinz, Cai-Na Hao, E. Montiel, Ramin A. Skibba, Alberto D. Bolatto, L. Vigroux, Alison F. Crocker, Sundar Srinivasan, C. D. Wilson, Eva Schinnerer, Oliver Krause, Daniela Calzetti, Frederick M. Walter, H-W. Rix, J. Dononvan Meyer, Sharon E. Meidt, Mark G. Wolfire, Daniel A. Dale, Nurur Rahman, Adam K. Leroy, Eric J. Murphy, Robert C. Kennicutt, G. Aniano
Publikováno v:
Publications of the Astronomical Society of the Pacific. 123:1347-1369
The KINGFISH project (Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel) is an imaging and spectroscopic survey of 61 nearby (d < 30 Mpc) galaxies, chosen to cover a wide range of galaxy properties and local interstellar medium (IS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::507d8c4799bd7d8e06b9c2a2af9f7a9e
https://doi.org/10.1086/663818
https://doi.org/10.1086/663818
Autor:
Ron Buta, A. Gil de Paz, J. L. Hinz, Eija Laurikainen, Heikki Salo, A. Bosma, Jarkko Laine, Martín Herrera-Endoqui, Karín Menéndez-Delmestre, Dimitri A. Gadotti, S. Comeron, J. H. Knapen, Benne W. Holwerda, E. Athanassoula, Michael W. Regan, Mark Seibert, Kartik Sheth, J. C. Muñoz-Mateoz, Luis C. Ho, T. Mizusawa, Tae Jung Kim, Santiago Erroz-Ferrer
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 562, ⟨10.1051/0004-6361/201321633⟩
Astronomy and Astrophysics-A&A, 2014, 562, ⟨10.1051/0004-6361/201321633⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 562, ⟨10.1051/0004-6361/201321633⟩
Astronomy and Astrophysics-A&A, 2014, 562, ⟨10.1051/0004-6361/201321633⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Resonance rings are the consequence of secular evolution processes that redistribute material and angular momentum in discs. We produced a Catalogue and an Atlas of the rings detected in the Spitzer Survey of Stellar Structure in Galaxies (S4G) and t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f8690509e0644f5f17287807ef97f780
https://hal.archives-ouvertes.fr/hal-01441021
https://hal.archives-ouvertes.fr/hal-01441021
Autor:
Sharon E. Meidt, Dennis Zaritsky, Jarkko Laine, S. Comeron, T. Mizusawa, Heikki Salo, Nor Pirzkal, J. H. Knapen, Benne W. Holwerda, Mark Seibert, J. L. Hinz, Michael W. Regan, Karín Menéndez-Delmestre, J. C. Muñoz-Mateos, Kartik Sheth, A. Gil-de-Paz, S. Erroz-Ferrer, A. Bosma, Seppo Laine, Eija Laurikainen, Dimitri A. Gadotti, Tae Jung Kim, Luis C. Ho, E. Athanassoula
Publikováno v:
ASTROPHYSICAL JOURNAL
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2014, 781 (1), ⟨10.1088/0004-637X/781/1/12⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
The Astrophysical Journal, 2014, 781 (1), ⟨10.1088/0004-637X/781/1/12⟩
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2014, 781 (1), ⟨10.1088/0004-637X/781/1/12⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
The Astrophysical Journal, 2014, 781 (1), ⟨10.1088/0004-637X/781/1/12⟩
International audience; The morphology of galaxies can be quantified to some degree using a set of scale-invariant parameters. Concentration (C), asymmetry (A), smoothness (S), the Gini index (G), the relative contribution of the brightest pixels to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::16b6464f2199279fdbd6c249398b8585
https://resolver.caltech.edu/CaltechAUTHORS:20140211-114726941
https://resolver.caltech.edu/CaltechAUTHORS:20140211-114726941
Autor:
Kevin V. Croxall, Eva Schinnerer, K. Kreckel, Robert C. Kennicutt, Fabian Walter, D. Calzetti, L. Armus, B. D. Johnson, Bernhard R. Brandl, Brent Groves, Maud Galametz, P. Beirao, Jd Smith, Karin Sandstrom, Daniel A. Dale, Jin Koda, L. K. Hunt, Eric W. Pellegrini, J. L. Hinz
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 777, 96
The Astrophysical Journal, 777, 96
The metal content of a galaxy, a key property for distinguishing between viable galaxy evolutionary scenarios, strongly influences many of the physical processes in the interstellar medium. An absolute and robust determination of extragalactic metall
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5ac115dee3dbb9d8f1699b09a3835d30
Autor:
L. K. Hunt, Eric J. Murphy, Marc Sauvage, P. N. Appleton, Eva Schinnerer, Fabian Walter, Stefano Zibetti, Karl D. Gordon, E. Montiel, H. W. Rix, K. V. Croxall, Bernhard R. Brandl, Karin Sandstrom, A. D. Bolatto, P. Beirao, Fatemeh Tabatabaei, D. Calzetti, H. Roussel, A. Crocker, L. Armus, C.-N. Hao, Sharon E. Meidt, Bruce T. Draine, George Helou, Brent Groves, Maud Galametz, N. Rahman, C. W. Engelbracht, A. E. Miller, J. L. Hinz, R. Skibba, Jd Smith, B. D. Johnson, Daniel A. Dale, Christine D. Wilson, G. Aniano, Adam K. Leroy, Robert C. Kennicutt, Jin Koda, Mark Wolfire, Oliver Krause, Yuexing Li
Publikováno v:
ASTROPHYSICAL JOURNAL
New far-infrared and sub-millimeter photometry from the Herschel Space Observatory is presented for 61 nearby galaxies from the Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel (KINGFISH) sample. The spatially-integrated fluxes ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e4099a61dc223b48cf0958685137543c
https://biblio.ugent.be/publication/8622864
https://biblio.ugent.be/publication/8622864
Autor:
C. W. Engelbracht, L. K. Hunt, R. A. Skibba, J. L. Hinz, D. Calzetti, K. D. Gordon, H. Roussel, A. F. Crocker, K. A. Misselt, A. D. Bolatto, R. C. Kennicutt, P. N. Appleton, L. Armus, P. Beirão, B. R. Brandl, K. V. Croxall, D. A. Dale, B. T. Draine, G. Dumas, A. Gil de Paz, B. Groves, C.-N. Hao, B. D. Johnson, J. Koda, O. Krause, A. K. Leroy, S. E. Meidt, E. J. Murphy, N. Rahman, H.-W. Rix, K. M. Sandstrom, M. Sauvage, E. Schinnerer, J.-D. T. Smith, S. Srinivasan, L. Vigroux, F. Walter, B. E. Warren, C. D. Wilson, M. G. Wolfire, S. Zibetti
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
ASTRONOMY & ASTROPHYSICS
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
instname
ASTRONOMY & ASTROPHYSICS
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Stellar density and bar strength should affect the temperatures of the cool (T ~ 20-30 K) dust component in the inner regions of galaxies, which implies that the ratio of temperatures in the circumnuclear regions to the disk should depend on Hubble t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e509ea6cb3e6db7254e6f3b5a4b3e906
https://eprints.ucm.es/35593/
https://eprints.ucm.es/35593/
Autor:
Karl D. Gordon, J. L. Hinz, Karl Misselt, Jane E. Morrison, Pablo G. Pérez-González, C. W. Engelbracht, George H. Rieke
Publikováno v:
AIP Conference Proceedings.
Spitzer provides substantial advances for studies of external galaxies: 1.) it has the very high sensitivity toward extended, low‐surface‐brightness sources made possible by a cryogenic telescope in space; 2.) the use of large format arrays and p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4bf2f8d21be4150a2d671ca71e2d2fe1
https://doi.org/10.1063/1.1913950
https://doi.org/10.1063/1.1913950
Autor:
A. Bosma, Dennis Zaritsky, Eija Laurikainen, Jarkko Laine, Kartik Sheth, Hélène M. Courtois, Dimitri A. Gadotti, Luis C. Ho, Mark Seibert, Jenny G. Sorce, Tae Jung Kim, Juan-Carlos Muñoz-Mateos, J. L. Hinz, S. Comeron, Santiago Erroz-Ferrer, Mauricio Cisternas, T. Mizusawa, Karín Menéndez-Delmestre, Benne W. Holwerda, Michael W. Regan, E. Athanassoula, A. Gil de Paz, Heikki Salo
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2014, 147, pp.134. ⟨10.1088/0004-6256/147/6/134⟩
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
instname
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2014, 147, pp.134. ⟨10.1088/0004-6256/147/6/134⟩
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
We combine data from the Spitzer Survey for Stellar Structure in Galaxies (S$^4$G), a recently calibrated empirical stellar mass estimator from Eskew et al., and an extensive database of HI spectral line profiles to examine the baryonic Tully-Fisher
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::35b0d02ddaed894710e95358220b5f5e
https://doi.org/10.1088/0004-6256/147/6/134
https://doi.org/10.1088/0004-6256/147/6/134
Autor:
D. A. Dale, D. O. Cook, H. Roussel, J. A. Turner, L. Armus, A. D. Bolatto, M. Boquien, M. J. I. Brown, D. Calzetti, I. De Looze, M. Galametz, K. D. Gordon, B. A. Groves, T. H. Jarrett, G. Helou, R. Herrera-Camus, J. L. Hinz, L. K. Hunt, R. C. Kennicutt, E. J. Murphy
Publikováno v:
Astrophysical Journal; 3/1/2017, Vol. 837 Issue 1, p1-1, 1p