Zobrazeno 1 - 8
of 8
pro vyhledávání: '"P. K. Humire"'
Autor:
Kunihiko Tanaka, Jeffrey G. Mangum, Serena Viti, Sergio Martín, Nanase Harada, Kazushi Sakamoto, Sebastien Muller, Yuki Yoshimura, Kouichiro Nakanishi, Rubén Herrero-Illana, Kimberly L. Emig, S. Mühle, Hiroyuki Kaneko, Tomoka Tosaki, Erica Behrens, Víctor M. Rivilla, Laura Colzi, Yuri Nishimura, P. K. Humire, Mathilde Bouvier, Ko-Yun Huang, Joshua Butterworth, David S. Meier, Paul P. van der Werf
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 1, p 18 (2024)
We present a spatially resolved excitation analysis for the central molecular zone (CMZ) of the starburst galaxy NGC 253 using the data from the Atacama Large Millimeter/submillimeter Array Comprehensive High-resolution Extragalactic Molecular Invent
Externí odkaz:
https://doaj.org/article/bf869a7ddf2443dbb7ec505bc43cc298
Autor:
Nanase Harada, Sergio Martín, Jeffrey G. Mangum, Kazushi Sakamoto, Sebastien Muller, Víctor M. Rivilla, Christian Henkel, David S. Meier, Laura Colzi, Mitsuyoshi Yamagishi, Kunihiko Tanaka, Kouichiro Nakanishi, Rubén Herrero-Illana, Yuki Yoshimura, P. K. Humire, Rebeca Aladro, Paul P. van der Werf, Kimberly L. Emig
Publikováno v:
The Astrophysical Journal, 938(1):80
The centers of starburst galaxies may be characterized by a specific gas and ice chemistry due to their gas dynamics and the presence of various ice desorption mechanisms. This may result in a peculiar observable composition. We analyse the abundance
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5f067af37f097c477784bbb5fffbc77
Autor:
P. K. Humire, C. Henkel, A. Hernández-Gómez, S. Martín, J. Mangum, N. Harada, S. Muller, K. Sakamoto, K. Tanaka, Y. Yoshimura, K. Nakanishi, S. Mühle, R. Herrero-Illana, D. S. Meier, E. Caux, R. Aladro, R. Mauersberger, S. Viti, L. Colzi, V. M. Rivilla, M. Gorski, K. M. Menten, K.-Y. Huang, S. Aalto, P. P. van der Werf, K. L. Emig
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 663, ⟨10.1051/0004-6361/202243384⟩
Astronomy & Astrophysics, 663:A33
Astronomy and Astrophysics-A&A, 2022, 663, ⟨10.1051/0004-6361/202243384⟩
Astronomy & Astrophysics, 663:A33
[Context] Methanol masers of Class I (collisionally pumped) and Class II (radiatively pumped) have been studied in great detail in our Galaxy in a variety of astrophysical environments such as shocks and star-forming regions and are they are helpful
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d1f5d55908a996c7a222b5c06b3a0ce2
https://hal-insu.archives-ouvertes.fr/insu-03867483
https://hal-insu.archives-ouvertes.fr/insu-03867483
Autor:
Erica Behrens, Jeffrey G. Mangum, Jonathan Holdship, Serena Viti, Nanase Harada, Sergio Martín, Kazushi Sakamoto, Sebastien Muller, Kunihiko Tanaka, Kouichiro Nakanishi, Rubén Herrero-Illana, Yuki Yoshimura, Rebeca Aladro, Laura Colzi, Kimberly L. Emig, Christian Henkel, Ko-Yun Huang, P. K. Humire, David S. Meier, Víctor M. Rivilla, Paul P. van der Werf
Publikováno v:
The Astrophysical Journal, 939(2):119
ALMA Comprehensive High-resolution Extragalactic Molecular Inventory (ALCHEMI) Collaboration.
We analyze HCN and HNC emission in the nearby starburst galaxy NGC 253 to investigate its effectiveness in tracing heating processes associated with st
We analyze HCN and HNC emission in the nearby starburst galaxy NGC 253 to investigate its effectiveness in tracing heating processes associated with st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f3027a84bf68868b5ce47c9f3b30a82a
https://ui.adsabs.harvard.edu/abs/2022ApJ...939..119B
https://ui.adsabs.harvard.edu/abs/2022ApJ...939..119B
Autor:
Nanase Harada, Sergio Martín, Jeffrey G. Mangum, Kazushi Sakamoto, Sebastien Muller, Kunihiko Tanaka, Kouichiro Nakanishi, Rubén Herrero-Illana, Yuki Yoshimura, Stefanie Mühle, Rebeca Aladro, Laura Colzi, Víctor M. Rivilla, Susanne Aalto, Erica Behrens, Christian Henkel, Jonathan Holdship, P. K. Humire, David S. Meier, Yuri Nishimura, Paul P. van der Werf, Serena Viti
Publikováno v:
The Astrophysical Journal, 923(1)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
Molecular abundances are sensitive to the UV photon flux and cosmic-ray ionization rate. In starburst environments, the effects of high-energy photons and particles are expected to be stronger. We examine these astrochemical signatures through multip
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::df43171c3714e292821ef86e6072d7db
http://hdl.handle.net/1887/3256712
http://hdl.handle.net/1887/3256712
Autor:
R. Mauersberger, D. Riquelme, A. Hernandez-Gomez, Jean-Christophe Loison, Arnaud Belloche, Karl M. Menten, V. Thiel, Christian Henkel, P. K. Humire, Thushara Pillai, Norbert Langer, Valentine Wakelam
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 642, pp.A222. ⟨10.1051/0004-6361/202038216⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 642, pp.A222. ⟨10.1051/0004-6361/202038216⟩
Measuring isotopic ratios is a sensitive technique used to obtain information on stellar nucleosynthesis and chemical evolution. We present measurements of the carbon and sulphur abundances in the interstellar medium of the central region of our Gala
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b54adac1ea2b4966e96ab94eff7a3b4e
https://hal.archives-ouvertes.fr/hal-02993705/document
https://hal.archives-ouvertes.fr/hal-02993705/document
Autor:
Xianming Chen, Simon Ellingsen, Y. Gong, S. A. Levshakov, Xindi Tang, Paola Castangia, Christian Henkel, A. Malawi, Benjamin Winkel, R. Mauersberger, T. P. McCarthy, H. Asiri, Silvia Leurini, P. K. Humire, Andrea Tarchi
Methanol (CH3OH) is one of the most abundant interstellar molecules, offering a vast number of transitions to be studied, including many maser lines. While the strongest Galactic CH3OH lines, the so-called class II masers, show no indications for the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c28aca72d80e71966800e3755e094c35
http://hdl.handle.net/20.500.12386/31374
http://hdl.handle.net/20.500.12386/31374
Autor:
Serena Viti, L. Colzi, Víctor M. Rivilla, Kazushi Sakamoto, P. van der Werf, P. K. Humire, K. Nakanishi, Carsten Henkel, K. L. Emig, Nanase Harada, Jonathan Holdship, Sergio Martín, Jeffrey G. Mangum, Santiago García-Burillo, Kunihiko Tanaka, S. Mühle, Rubén Herrero-Illana, Yuki Yoshimura, Rebeca Aladro, David S. Meier, Sebastien Muller
Publikováno v:
Astronomy & Astrophysics, 654, 1-18
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
[Context] Observations of chemical species can provide insights into the physical conditions of the emitting gas however it is important to understand how their abundances and excitation vary within different heating environments. C2H is a molecule t