Zobrazeno 1 - 10
of 216
pro vyhledávání: '"J. T. Moore"'
Autor:
Geumsook Park, Malcolm J. Currie, Holly S. Thomas, Erik Rosolowsky, Jessica T. Dempsey, Kee-Tae Kim, Andrew J. Rigby, Yang Su, David J. Eden, Dario Colombo, Harriet Parsons, Toby J. T. Moore
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 264, Iss 1, p 16 (2022)
We present the full data release of the ^12 CO (3–2) High-Resolution Survey (COHRS), which has mapped the inner Galactic plane over the range of 9.°5 ≤ l ≤ 62.°3 and ∣ b ∣ ≤ 0.°5. COHRS has been carried out using the Heterodyne Array R
Externí odkaz:
https://doaj.org/article/1e7af6fc0c75439894cf68108f72e4d8
Autor:
M R A Wells, J S Urquhart, T J T Moore, K E Browning, S E Ragan, A J Rigby, D J Eden, M A Thompson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 516:4245-4255
The ATLASGAL survey has characterised the properties of approximately 1000 embedded HII regions and found an empirical relationship between the clump mass and bolometric luminosity that covers 3-4 orders of magnitude. Comparing this relation with sim
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 515:271-285
It is speculated that the high star-formation efficiency observed in spiral-arm molecular clouds is linked to the prevalence of compressive (curl-free) turbulent modes, while the shear-driven solenoidal (divergence-free) modes appear to be the main c
Autor:
Raffaele Rani, Toby J T Moore, David J Eden, Andrew J Rigby, Ana Duarte-Cabral, Yueh-Ning Lee
The growing range of automated algorithms for the identification of molecular clouds and clumps in large observational datasets has prompted the need for the direct comparison of these procedures. However, these methods are complex and testing for bi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c0ea7c15684b0ccc223f255c1842b40e
Publikováno v:
Journal of Cultural Heritage. 35:218-224
Synthetic organic pigments have been used in works of art for well over 130 years. During this time, many have been introduced and some have been removed from production. Historical pigments are synthetic organic pigments that are no longer commercia
Autor:
Timea Csengeri, Leonardo Testi, Andrew Rigby, Karl M. Menten, S. J. Billington, V. S. Veena, Erik Muller, Friedrich Wyrowski, Alessio Traficante, M. T. Beltrán, Peter Schilke, S. Leurini, K. Torstensson, Jens Kauffmann, Toby J. T. Moore, M-Y Lee, Adam Ginsburg, P. Venegas, S-N X. Medina, Sylvain Bontemps, Frederic Schuller, D. Russeil, Leonardo Bronfman, Ke Wang, Sümeyye Suri, Riccardo Cesaroni, S. Lopez, David Eden, P. Mazumdar, F. Azagra, Th. Henning, Dario Colombo, Sarah Ragan, Jouni Kainulainen, P. J. Barnes, M. Wienen, M. Riener, Sergio Molinari, Álvaro Sánchez-Monge, Audra K. Hernandez, James Urquhart, A. Giannetti, F. M. Montenegro-Montes, Eugenio Schisano, Annie Zavagno, Rodrigo Parra, Frédérique Motte, M. Mattern, Alex R. Pettitt, Henrik Beuther, Clare Dobbs, Nicola Schneider, F. Mac-Auliffe, C. Agurto, E. Gonzalez, L. D. Anderson, Q. Nguyen-Luong, Ricardo Finger, J-P Perez-Beaupuits, Ana Duarte-Cabral
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 500 (3), pp.3064-3082. ⟨10.1093/mnras/staa2369⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 500 (3), pp.3064-3082. ⟨10.1093/mnras/staa2369⟩
The SEDIGISM (Structure, Excitation and Dynamics of the Inner Galactic Interstellar Medium) survey used the APEX telescope to map 84 deg^2 of the Galactic plane between l = -60 deg and l = +31 deg in several molecular transitions, including 13CO(2-1)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bc160a4e4b9d5d2bd0b80def20f8cd6a
https://hal.archives-ouvertes.fr/hal-03046462
https://hal.archives-ouvertes.fr/hal-03046462
Autor:
K. A. Marsh, D. Johnstone, K. Tahani, Andrew Rigby, Paul C. Clark, Sarah Ragan, Rene Plume, Mark Thompson, David Eden, James Urquhart, C. H. Peñaloza, Toby J. T. Moore, Harriet Parsons, R. Rani, Matthew Smith
We have used the ratio of column densities (CDR) derived independently from the 850-$\mu$m continuum JCMT Plane Survey (JPS) and the $^{13}$CO/C$^{18}$O $(J=3-2)$ Heterodyne Inner Milky Way Plane Survey (CHIMPS) to produce maps of the dense-gas mass
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f85824002fac517de42556ae80ccfe5b
https://resolver.caltech.edu/CaltechAUTHORS:20210114-164620647
https://resolver.caltech.edu/CaltechAUTHORS:20210114-164620647
Autor:
Cinthya N. Herrera, Dario Colombo, Frank Bigiel, Annie Hughes, M. Querejeta, Andrew Rigby, Santiago García-Burillo, Eva Schinnerer, Sharon Meidt, Toby J. T. Moore, C. G. Mundell, Ute Lisenfeld, Federico Lelli, J. M. D. Kruijssen, Jérôme Pety
Publikováno v:
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Digibug: Repositorio Institucional de la Universidad de Granada
Universidad de Granada (UGR)
Astronomy & Astrophysics
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A97. ⟨10.1051/0004-6361/202038955⟩
instname
Digibug: Repositorio Institucional de la Universidad de Granada
Universidad de Granada (UGR)
Astronomy & Astrophysics
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A97. ⟨10.1051/0004-6361/202038955⟩
Tidal dwarf galaxies (TDGs) are gravitationally bound condensations of gas and stars that formed during galaxy interactions. Here we present multi-configuration ALMA observations of J1023+1952, a TDG in the interacting system Arp 94, where we resolve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d1e1f9abec06474891b451f305834d12
http://hdl.handle.net/10481/67199
http://hdl.handle.net/10481/67199
Autor:
Sarah Ragan, M. Riener, Nicola Schneider, M. T. Beltrán, L. D. Anderson, Ke Wang, S. N. X. Medina, S. Lopez, Andrew Rigby, Adam Ginsburg, P. Venegas, F. M. Montenegro-Montes, Frédérique Motte, Rodrigo Parra, Ricardo Finger, Annie Zavagno, M. Wienen, D. Russeil, Andrea Giannetti, Henrik Beuther, Karl M. Menten, Erik Muller, Álvaro Sánchez-Monge, C. Agurto, M. Mattern, Toby J. T. Moore, F. Mac-Auliffe, Silvia Leurini, Jens Kauffmann, Sergio Molinari, James Urquhart, V. S. Veena, Timea Csengeri, Alberto Sanna, P. Mazumdar, E. Gonzalez, L. Testi, Leonardo Bronfman, Min-Young Lee, Q. Nguyen-Luong, Ana Duarte-Cabral, Clare Dobbs, Jouni Kainulainen, Alessio Traficante, Peter Schilke, Th. Henning, Dario Colombo, J. P. Pérez-Beaupuits, Friedrich Wyrowski, K. Torstensson, Audra K. Hernandez, Sylvain Bontemps, Frederic Schuller, P. J. Barnes, Eugenio Schisano, David Eden, Riccardo Cesaroni, F. Azagra, Sümeyye Suri, Alex R. Pettitt
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 500 (3), pp.3027-3049. ⟨10.1093/mnras/staa2480⟩
Monthly Notices of the Royal Astronomical Society, 2021, 500 (3), pp.3027-3049. ⟨10.1093/mnras/staa2480⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 500 (3), pp.3027-3049. ⟨10.1093/mnras/staa2480⟩
Monthly Notices of the Royal Astronomical Society, 2021, 500 (3), pp.3027-3049. ⟨10.1093/mnras/staa2480⟩
We use the 13CO(2-1) emission from the SEDIGISM high-resolution spectral-line survey of the inner Galaxy, to extract the molecular cloud population with a large dynamic range in spatial scales, using the SCIMES algorithm. This work compiles a cloud c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::60151acf5371e870a430a6cb82e292a9
http://arxiv.org/abs/2012.01502
http://arxiv.org/abs/2012.01502
Autor:
J. Campbell-White, W.-J. Kim, Karl M. Menten, S. J. Billington, Toby J. T. Moore, Simon Ellingsen, Shari Breen, Silvia Leurini, David Eden, C. König, Henrik Beuther, Mark Thompson, James Urquhart
Publikováno v:
Monthly Notices of the Royal Astronomical Society
We have used catalogues from several Galactic plane surveys and dedicated observations to investigate the relationship between various maser species and Galactic star forming clumps, as identified by the ATLASGAL survey. The maser transitions of inte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9e9c365c7216c524fa51caaa1ef64274
https://eprints.whiterose.ac.uk/188764/1/staa2936.pdf
https://eprints.whiterose.ac.uk/188764/1/staa2936.pdf