Zobrazeno 1 - 10
of 228
pro vyhledávání: '"L. D. Anderson"'
Autor:
L. D. Anderson, Matteo Luisi, B. Liu, Dylan J. Linville, Robert A. Benjamin, Natasha Hurley-Walker, N. M. McClure-Griffiths, Catherine Zucker
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 1, p 43 (2024)
The Galactic center lobe (GCL) is an object ∼1° across that is located north of the Galactic center. In the mid-infrared (MIR) the GCL appears as two 8.0 μ m filaments between which there is strong 24 μ m and radio continuum emission. Due to its
Externí odkaz:
https://doaj.org/article/546719e959124933b965be88edc6106b
Autor:
Natasha Hurley-Walker, L. D. Anderson, M. Luisi, N. M. McClure-Griffiths, Robert A. Benjamin, Michael A. Kuhn, Dylan J. Linville, B. Liu, Catherine Zucker
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 1, p 42 (2024)
The Galactic center lobe (GCL) is a ∼1° object located north of the Galactic center. In the mid-infrared, the GCL appears as two 8.0 μ m filaments that roughly define an ellipse. There is strong 24 μ m and radio continuum emission in the interio
Externí odkaz:
https://doaj.org/article/71e11db08c38490aaf8598b4def8c9e9
Autor:
Dylan J. Linville, Matteo Luisi, L. D. Anderson, Bin Liu, T. M. Bania, Dana S. Balser, Trey V. Wenger, L. M. Haffner, J. L. Mascoop
Publikováno v:
The Astrophysical Journal, Vol 959, Iss 2, p 110 (2023)
The Green Bank Telescope Diffuse Ionized Gas Survey (GDIGS) traces ionized gas in the Galactic midplane by observing radio recombination line (RRL) emission from 4 to 8 GHz. The nominal survey zone is 32.°3 > ℓ > −5°, ∣ b ∣ < 0.°5. Here, w
Externí odkaz:
https://doaj.org/article/7fd8f5723c6b4f879a1f46978dd1a2fe
Autor:
C. Rodriguez, J. L. Kaufman, J. Laubach, D. W. Sborov, B. Reeves, A. Chari, R. Silbermann, L. J. Costa, L. D. Anderson, Jr, N. Nathwani, N. Shah, N. Bumma, A. Jakubowiak, R. Z. Orlowski, H. Pei, A. Cortoos, S. Patel, T. S. Lin, P. G. Richardson, P. M. Voorhees
Publikováno v:
HemaSphere, Vol 6, Pp 824-825 (2022)
Externí odkaz:
https://doaj.org/article/0442f51585344f1c92f26b43f2f47796
Autor:
R. Dokara, Y. Gong, W. Reich, M. R. Rugel, A. Brunthaler, K. M. Menten, W. D. Cotton, S. A. Dzib, S. Khan, S.-N. X. Medina, H. Nguyen, G. N. Ortiz-León, J. S. Urquhart, F. Wyrowski, A. Y. Yang, L. D. Anderson, H. Beuther, T. Csengeri, P. Müller, J. Ott, J. D. Pandian, N. Roy
Publikováno v:
Astronomy & Astrophysics. 671:A145
Context. While over 1000 supernova remnants (SNRs) are estimated to exist in the Milky Way, only less than 400 have been found to date. In the context of this apparent deficiency, more than 150 SNR candidates were recently identified in the D-configu
Autor:
Volker Ossenkopf-Okada, Christof Buchbender, Nicola Schneider, Rebeca Aladro, Matteo Luisi, Maria S. Kirsanova, A. M. Sobolev, M. R. Samal, Paul A. Boley, L. D. Anderson, John H. Bieging, Yoko Okada, Morten Andersen, Ya. N. Pavlyuchenkov
Publikováno v:
Mon. Not. R. Astron. Soc.
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
The aim of the present work is to study structure and gas kinematics in the photodissociation regions (PDRs) around the compact HII regions S235A and S235C. We observe the [CII], [13CII] and [OI] line emission, using SOFIA/upGREAT and complement them
Autor:
Alessio Traficante, Andrew Rigby, Timea Csengeri, Karl M. Menten, James Urquhart, K. R. Neralwar, Th. Henning, Friedrich Wyrowski, Álvaro Sánchez-Monge, Peter J. Barnes, Leonardo Bronfman, David Eden, S.-N. X. Medina, Henrik Beuther, M. Mattern, Alex R. Pettitt, Allen Y. Yang, L. D. Anderson, Adam Ginsburg, Frederic Schuller, M.-Y. Lee, Ana Duarte-Cabral, Sarah Ragan, M. Wienen, D. Colombo, C. König
The morphology of the Milky Way is still a matter of debate. In order to shed light on uncertainties surrounding the structure of the Galaxy, in this paper, we study the imprint of spiral arms on the distribution and properties of its molecular gas.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c04f4a6476a98e7b095cf0d48f8a75f2
https://hal-insu.archives-ouvertes.fr/insu-03439581
https://hal-insu.archives-ouvertes.fr/insu-03439581
Autor:
J. Wallace, C. Battersby, E. A. C. Mills, J. D. Henshaw, M. C. Sormani, A. Ginsburg, A. T. Barnes, H. P. Hatchfield, S. C. O. Glover, L. D. Anderson
Publikováno v:
The Astrophysical Journal. 939:58
We report on the discovery of linear filaments observed in CO(1-0) emission for a $\sim2'$ field of view toward the Sgr E star forming region centered at (l,b)=(358.720$^\circ$, 0.011$^\circ$). The Sgr E region is thought to be at the turbulent inter
Autor:
W. P. Armentrout, L. D. Anderson, Joanne Dawson, T. M. Bania, Trey V. Wenger, John M. Dickey, Dana S. Balser, Christopher H. Jordan, Naomi McClure-Griffiths
The Southern HII Region Discovery Survey (SHRDS) is a 900 hour Australia Telescope Compact Array 4-10 GHz radio continuum and radio recombination line (RRL) survey of Galactic HII regions and infrared-identified HII region candidates in the southern
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd5a8be2331998913580e328b1f09918
https://doi.org/10.3847/1538-4365/abf4d4
https://doi.org/10.3847/1538-4365/abf4d4
Autor:
Valentin D. Ivanov, Phil Lucas, L. D. Anderson, Zhen Guo, Robert A. Benjamin, André-Nicolas Chené, Danilo Gonzalez, Christian Moni Bidin, Sebastian Ramírez-Alegría, Leigh C. Smith, Karla Peña Ramírez, Artemio Herrero, Jura Borissova, Radostin Kurtev, W. P. Armentrout, Carlos González-Fernández, F. Mauro, Dante Minniti
We have investigated the stellar and interstellar content of the distant star formation region IRAS 17591-2228 (WISE HII region GAL 007.47+0.06). It is associated to a water maser, whose parallax distance is d=20.4^{+2.8} {-2.2} kpc, supported by ind
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::91514aad430ecbd20650f4146325328a
http://arxiv.org/abs/2103.05849
http://arxiv.org/abs/2103.05849