Zobrazeno 1 - 10
of 91
pro vyhledávání: '"lines and bands [ISM]"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Lukas J Furtak, Adèle Plat, Adi Zitrin, Micheal W Topping, Daniel P Stark, Victoria Strait, Stéphane Charlot, Dan Coe, Felipe Andrade-Santos, Maruša Bradač, Larry Bradley, Brian C Lemaux, Keren Sharon
Publikováno v:
Furtak, L J, Plat, A, Zitrin, A, Topping, M W, Stark, D P, Strait, V, Charlot, S, Coe, D, Andrade-Santos, F, Bradac, M, Bradley, L, Lemaux, B C & Sharon, K 2022, ' A double-peaked Lyman-alpha emitter with a stronger blue peak multiply imaged by the galaxy cluster RXC J0018.5+1626 ', Monthly Notices of the Royal Astronomical Society, vol. 516, no. 1, pp. 1373-1385 . https://doi.org/10.1093/mnras/stac2169
We report the discovery of a double-peaked Lyman-$\alpha$ (Ly$\alpha$) emitter (LAE) at $z=3.2177\pm0.0001$ in VLT/MUSE data. The galaxy is strongly lensed by the galaxy cluster RXC~J0018.5+1626 recently observed in the RELICS survey, and the double-
Autor:
Gaia collaboration, Schultheis, M., Zhao, H., Zwitter, T., Marshall, D. J., Drimmel, R., Frémat, Y., Bailer-Jones, C. A. L., Recio-Blanco, A., Kordopatis, G., de Laverny, P., Andrae, R., Dharmawardena, T. E., Fouesneau, M., Sordo, R.
Publikováno v:
Astronomy & Astrophysics
Astronomy & Astrophysics, 674, pp. 1-25
Davidson, M, Hambly, N C, Mann, R G, Morris, D & Rowell, N & Voutsinas, S 2023, ' Gaia Data Release 3. Exploring and mapping the diffuse interstellar band at 862 nm ', Astronomy and Astrophysics, vol. 674, A40, pp. 1-25 . https://doi.org/10.1051/0004-6361/202243283
Astronomy & Astrophysics, 674, pp. 1-25
Davidson, M, Hambly, N C, Mann, R G, Morris, D & Rowell, N & Voutsinas, S 2023, ' Gaia Data Release 3. Exploring and mapping the diffuse interstellar band at 862 nm ', Astronomy and Astrophysics, vol. 674, A40, pp. 1-25 . https://doi.org/10.1051/0004-6361/202243283
Diffuse interstellar bands (DIBs) are common interstellar absorption features in spectroscopic observations but their origins remain unclear. DIBs play an important role in the life cycle of the interstellar medium (ISM) and can also be used to trace
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universitat Pompeu Fabra
Universitat Pompeu Fabra
This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model) We have detected a b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::a230d25eb9ff396cb745c331443e1aa4
https://hdl.handle.net/20.500.12666/545
https://hdl.handle.net/20.500.12666/545
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
28 pags., 21 figs., 9 tabs. -- This paper is dedicated to the memory of Bruce Swinyard, for his mentorship and his major contributions to the SPIRE-FTS performance and calibration.
Context. Star-forming galaxies emit bright molecular and atomic
Context. Star-forming galaxies emit bright molecular and atomic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b2523113b7ff02b4df571fc5562b9854
http://hdl.handle.net/10261/258525
http://hdl.handle.net/10261/258525
Autor:
Martin A. Barstow, V. Schaffenroth, Sarah L. Casewell, Nicole Reindl, M. M. Miller Bertolami, S. Taubenberger, Nicolle L. Finch, Stephan Geier
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The nucleus of the planetary nebula Hen2-428 is a short orbital-period (4.2h), double-lined spectroscopic binary, whose status as a potential supernova type Ia progenitor has raised some controversy in the literature. With the aim of resolving this d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9b3f9ddcf4f5bfe08d12143d43f5d5ca
https://www.aanda.org/10.1051/0004-6361/202038117
https://www.aanda.org/10.1051/0004-6361/202038117
Autor:
Belén Tercero, P. de Vicente, José Cernicharo, Nuria Marcelino, Carlos Cabezas, Juan R. Pardo, Marcelino Agúndez, Celina Bermúdez
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
9 pags., 6 figs., 7 tabs., 1 app.
We report on the first detection of C3N- and C5N- towards the cold dark core TMC-1 in the Taurus region, using the Yebes 40 m telescope. The observed C3N/C3N- and C5N/C5N- abundance ratios are ∼140 and ∼2, r
We report on the first detection of C3N- and C5N- towards the cold dark core TMC-1 in the Taurus region, using the Yebes 40 m telescope. The observed C3N/C3N- and C5N/C5N- abundance ratios are ∼140 and ∼2, r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef1c57c262df118ac49c14527ff01097
Publikováno v:
Popping, G, Narayanan, D, Somerville, R S, Faisst, A L & Krumholz, M R 2019, ' The art of modelling CO, [C I], and [C II] in cosmological galaxy formation models ', Monthly Notices of the Royal Astronomical Society, vol. 482, no. 4, pp. 4906-4932 . https://doi.org/10.1093/mnras/sty2969
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
The advent of new sub-millimeter observational facilities has stimulated the desire to model the sub-mm line emission of galaxies within cosmological galaxy formation models. This is typically done in post-processing by applying sub-resolution recipe
Autor:
Elisabetta Valiante, Asantha Cooray, Edo Ibar, Simon Dye, D. J. B. Smith, E. van Kampen, Sébastien Viaene, Rob Ivison, Manuel Aravena, Luke J. M. Davies, V. Villanueva, Michał J. Michałowski, Steve Maddox, Maritza A. Lara-López, Simon P. Driver, Ivan Oteo, C. Furlanetto, Matthew Smith, Yongquan Xue, Rodrigo Herrera-Camus, Maarten Baes, Stephen Anthony Eales, Loretta Dunne, P. van der Werf, Nathan Bourne, T. M. Hughes
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (ISSN 0035-8711), 468(1), L103-L107
ResearcherID
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (ISSN 0035-8711), 468(1), L103-L107
ResearcherID
We present the calibration between the dust continuum luminosity and interstellar gas content obtained from the Valpara\'{i}so ALMA Line Emission Survey (VALES) sample of 67 main-sequence star-forming galaxies at 0.02
Comment: Accepted for publi
Comment: Accepted for publi
Publikováno v:
Gray, M D, Baggott, J, Westlake, J & Etoka, S 2019, ' Maser flare simulations from oblate and prolate clouds ', Monthly Notices of the Royal Astronomical Society, vol. 486, no. 3, pp. 4216-4225 . https://doi.org/10.1093/mnras/stz1137
We investigated, through numerical models, the flaring variability that may arise from the rotation of maser clouds of approximately spheroidal geometry, ranging from strongly oblate to strongly prolate examples. Inversion solutions were obtained for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b490b7490daf6b1ecbeea384d2f18928
http://arxiv.org/abs/1904.10347
http://arxiv.org/abs/1904.10347