Zobrazeno 1 - 10
of 94
pro vyhledávání: '"Jorge L. Pineda"'
Autor:
Jin Koda, Akihiko Hirota, Fumi Egusa, Kazushi Sakamoto, Tsuyoshi Sawada, Mark Heyer, Junichi Baba, Samuel Boissier, Daniela Calzetti, Jennifer Donovan Meyer, Bruce G. Elmegreen, Armando Gil de Paz, Nanase Harada, Luis C. Ho, Masato I. N. Kobayashi, Nario Kuno, Amanda M Lee, Barry F. Madore, Fumiya Maeda, Sergio Martín, Kazuyuki Muraoka, Kouichiro Nakanishi, Sachiko Onodera, Jorge L. Pineda, Nick Scoville, Yoshimasa Watanabe
Publikováno v:
The Astrophysical Journal, Vol 949, Iss 2, p 108 (2023)
We present Atacama Large Millimeter/submillimeter Array (ALMA) imaging of molecular gas across the full star-forming disk of the barred spiral galaxy M83 in CO( J = 1–0). We jointly deconvolve the data from ALMA’s 12 m, 7 m, and Total Power array
Externí odkaz:
https://doaj.org/article/7035afd7afc94d549c978f60e9d55ac2
Autor:
Matthew E Orr, Blakesley Burkhart, Andrew Wetzel, Philip F Hopkins, Ivanna A Escala, Allison L Strom, Paul F Goldsmith, Jorge L Pineda, Christopher C Hayward, Sarah R Loebman
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:3708-3726
We examine the azimuthal variations in gas-phase metallicity profiles in simulated Milky Way-mass disc galaxies from the Feedback in Realistic Environments (FIRE-2) cosmological zoom-in simulation suite, which includes a sub-grid turbulent metal mixi
Autor:
Mansi Padave, Rolf A. Jansen, Dylan Nelson, Hansung B. Gim, Guinevere Kauffmann, Sanchayeeta Borthakur, Timothy M. Heckman, David A. Thilker, Robert C. Kennicutt, Jorge L. Pineda, Andrew J. Fox, Jason Tumlinson, Emmanuel Momjian
We report the discovery of two kinematically anomalous atomic hydrogen (HI) clouds in M 100 (NGC 4321), which was observed as part of the Deciphering the Interplay between the Interstellar medium, Stars, and the Circumgalactic medium (DIISC) survey i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f31f7884cf2a2d18299cd9d89c42c0ab
http://arxiv.org/abs/2109.06247
http://arxiv.org/abs/2109.06247
Autor:
Melissa Soriano, Kristen Virkler, Jorge L. Pineda, Brian Bradford, Shinji Horiuchi, Tyrone McNichols, Jonathon Kocz
Publikováno v:
2021 XXXIVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS).
The Deep Space Network (DSN) enables NASA to communicate with its deep space spacecraft. By virtue of its large antennas, the DSN can be used as a powerful instrument for radio astronomy. In particular, Deep Space Station (DSS) 43, the 70 m antenna a
We present polarimetric observations of the Keyhole Nebula in the Carina Nebula Complex carried out using the Stratospheric Observatory for Infrared Astronomy. The Keyhole Nebula located to the west of $\eta$ Carinae is believed to be disturbed by th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a21cc444232079760a6b825a4e070010
http://arxiv.org/abs/2106.11364
http://arxiv.org/abs/2106.11364
Publikováno v:
Revista Cubana de Cirugía, Vol 39, Iss 1, Pp 68-72 (2000)
Se analizaron los resultados del tratamiento quirúrgico electivo de la úlcera duodenal con la vagotomía altamente selectiva (VAS) y la vagotomía troncular más piloroplastia (VT + P) en el Hospital Militar Central "Dr. Carlos J. Finlay", durante
Externí odkaz:
https://doaj.org/article/46c628e59a41438cab9ee42569f1c5d7
Autor:
Philip F. Hopkins, Jorge L. Pineda, Matthew E. Orr, Andrew Wetzel, Anne M. Medling, Alexander B. Gurvich, Kung-Yi Su, Dušan Kereš, Christopher C. Hayward, Claude André Faucher-Giguère, Norman Murray
Publikováno v:
Monthly Notices of the Royal Astronomical Society, vol 496, iss 2
We study the spatially resolved (sub-kpc) gas velocity dispersion ($\sigma$)--star formation rate (SFR) relation in the FIRE-2 (Feedback in Realistic Environments) cosmological simulations. We specifically focus on Milky Way mass disk galaxies at lat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f54c8cbb5a3b7f50df2622bf6e9e2966
https://escholarship.org/uc/item/9c80z2rb
https://escholarship.org/uc/item/9c80z2rb
Autor:
Sergio Molinari, Hendrik Linz, Jerome Amiaux, Floris van der Tak, Marc Sauvage, Frank Helmich, Divya Bhatia, Javier R. Goicoechea, Volker Ossenkopf-Okada, Jorge L. Pineda, Matthias Lezius, Martina C. Wiedner, Henrik Beuther, Luisa Buinhas, Eva Schinnerer, Roger Förstner, Oliver Krause, Maryvonne Gerin, Yao Liu, Urs U. Graf, Gilles Durand
Publikováno v:
Experimental Astronomy
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
37 pags., 12 figs., 1 tab.
The far-infrared (FIR) regime is one of the wavelength ranges where no astronomical data with sub-arcsecond spatial resolution exist. None of the medium-term satellite projects like SPICA, Millimetron, or the Origins S
The far-infrared (FIR) regime is one of the wavelength ranges where no astronomical data with sub-arcsecond spatial resolution exist. None of the medium-term satellite projects like SPICA, Millimetron, or the Origins S
Autor:
Christian Fischer, Jorge L. Pineda, Ralf S. Klessen, Paul F. Goldsmith, Simon C. O. Glover, Jürgen Stutzki, Robin G. Treß, Rowan J. Smith, Christof Buchbender, Bhaswati Mookerjea, Jin Koda, Monika Ziebart, Carsten Kramer
We present the first complete, velocity-resolved [CII] 158um image of the M51 grand-design spiral galaxy, observed with the upGREAT instrument on SOFIA. [CII] is an important tracer of various phases of the interstellar medium (ISM), including ionize
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7cb01aa816611291df8a04bc0a1f6bfd
Autor:
Fabio P. Santos, Leslie W. Looney, Ian W. Stephens, Edward J. Wollack, John E. Vaillancourt, Konstantinos Tassis, Alex Lazarian, David T. Chuss, Thomas Henning, Mark Morris, Derek Ward-Thompson, Doyal A. Harper, Dominic J. Benford, Gordon J. Stacey, Ellen G. Zweibel, C. Darren Dowell, Kartik Sheth, Marc Berthoud, Giles Novak, Joseph M. Michail, Jin-Ah Kim, Javad Siah, Shaul Hanany, Terry Jay Jones, Daniel A. Dale, Jorge L. Pineda, Laura M. Fissel, Christopher Q. Trinh, Johannes Staguhn, Michael W. Werner, Paul F. Goldsmith, Ryan T. Hamilton
SOFIA HAWC+ polarimetry at $154~\micron$ is reported for the face-on galaxy M51 and the edge-on galaxy NGC 891. For M51, the polarization vectors generally follow the spiral pattern defined by the molecular gas distribution, the far-infrared (FIR) in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0350df980e6135f9877dddcb477f8e7a