Zobrazeno 1 - 10
of 143
pro vyhledávání: '"S R Federman"'
Autor:
Adam M. Ritchey, Edward B. Jenkins, J. Michael Shull, Blair D. Savage, S. R. Federman, David L. Lambert
Publikováno v:
The Astrophysical Journal, Vol 952, Iss 1, p 57 (2023)
In this investigation, we present an analysis of the metallicity distribution that pertains to neutral gas in the local Galactic interstellar medium (ISM). We derive relative ISM metallicities for a sample of 84 sight lines probing diffuse atomic and
Externí odkaz:
https://doaj.org/article/390ef8b3981d47dc81f5326b52814f91
Publikováno v:
The Astrophysical Journal, Vol 948, Iss 2, p 139 (2023)
We present a comprehensive examination of interstellar P and Cl abundances based on an analysis of archival spectra acquired with the Space Telescope Imaging Spectrograph of the Hubble Space Telescope and the Far Ultraviolet Spectroscopic Explorer. C
Externí odkaz:
https://doaj.org/article/4cbc4bb9605e47ff9a04a6a1343e35a1
Autor:
Zhongxing, Xu, S R, Federman, William M, Jackson, Cheuk-Yiu, Ng, Lee-Ping, Wang, Kyle N, Crabtree
Publikováno v:
The Journal of chemical physics. 157(2)
Photodissociation is one of the main destruction pathways for dicarbon (C
Publikováno v:
Cerâmica, Vol 55, Iss 335, Pp 257-262 (2009)
Foi obtido um filme bioativo sol-gel do sistema SiO2-CaO através da mistura de precursor de silício (TEOS - tetraetil ortosilicato), precursor de cálcio (nitrato de cálcio tetrahidratado) e álcool em meio ácido. Após a mistura, a solução ser
Externí odkaz:
https://doaj.org/article/859a5e47952e4a58860e4dbb13e70380
Publikováno v:
Cerâmica, Vol 55, Iss 334, Pp 177-180 (2009)
Foi preparado um filme bioativo do sistema SiO2-CaO-P2O5 via sol-gel pela hidrólise e condensação de TEOS, TEP, álcool e nitrato de cálcio em meio ácido. Após a mistura, a solução sintetizada serviu para revestir substrato de aço inoxidáve
Externí odkaz:
https://doaj.org/article/b1a6008f5fdc476bb7b4963641bed637
Autor:
S. R. Federman, Johnathan S. Rice, John H. Lacy, Adam M. Ritchey, Nicolas Flagey, David L. Lambert, Gregory N. Mace, Paul F. Goldsmith, Hwihyun Kim
We study four lines of sight that probe the transition from diffuse molecular gas to molecular cloud material in Taurus. Measurements of atomic and molecular absorption are used to infer the distribution of species and the physical conditions toward
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0e42df26bf1739d5543d5add8d9fabc6
http://arxiv.org/abs/2106.12748
http://arxiv.org/abs/2106.12748
Autor:
Rafał Hakalla, S. R. Federman, M. Niu, Joël Lemaire, M. Eidelsberg, N. de Oliveira, A. N. Heays, R. W. Field, Wim Ubachs, James R. Lyons, Edcel J. Salumbides, G. Stark
Publikováno v:
Journal of Quantitative Spectroscopy and Radiative Transfer
Journal of Quantitative Spectroscopy and Radiative Transfer, Elsevier, 2017, 189, pp.312-328. ⟨10.1016/j.jqsrt.2016.12.012⟩
Journal of Quantitative Spectroscopy and Radiative Transfer, 189, 312-328. Elsevier Limited
Hakalla, R, Niu, M L, Field, R W, Heays, A N, Salumbides, E J, Stark, G, Lyons, J R, Eidelsberg, M, Lemaire, J L, Federman, S R, de Oliveira, N & Ubachs, W 2017, ' Fourier-transform spectroscopy of 13 C 17 O and deperturbation analysis of the A 1 Π (υ=0–3) levels ', Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 189, pp. 312-328 . https://doi.org/10.1016/j.jqsrt.2016.12.012
Journal of Quantitative Spectroscopy and Radiative Transfer, 2017, 189, pp.312-328. ⟨10.1016/j.jqsrt.2016.12.012⟩
Journal of Quantitative Spectroscopy and Radiative Transfer, Elsevier, 2017, 189, pp.312-328. ⟨10.1016/j.jqsrt.2016.12.012⟩
Journal of Quantitative Spectroscopy and Radiative Transfer, 189, 312-328. Elsevier Limited
Hakalla, R, Niu, M L, Field, R W, Heays, A N, Salumbides, E J, Stark, G, Lyons, J R, Eidelsberg, M, Lemaire, J L, Federman, S R, de Oliveira, N & Ubachs, W 2017, ' Fourier-transform spectroscopy of 13 C 17 O and deperturbation analysis of the A 1 Π (υ=0–3) levels ', Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 189, pp. 312-328 . https://doi.org/10.1016/j.jqsrt.2016.12.012
Journal of Quantitative Spectroscopy and Radiative Transfer, 2017, 189, pp.312-328. ⟨10.1016/j.jqsrt.2016.12.012⟩
The high-resolution B$^1\Sigma^+$ - A$^1\Pi$ (0, 0) and (0, 3) emission bands of the less-abundant $^{13}$C$^{17}$O isotopologue have been investigated by Fourier-transform spectroscopy in the visible region using a Bruker IFS 125HR spectrometer at a
Autor:
M. L. Niu, Joël Lemaire, S. R. Federman, Rafał Hakalla, Alan N. Heays, M. Eidelsberg, James R. Lyons, N. de Oliveira, Wim Ubachs, G. Stark, Izabela Piotrowska, R. Kępa, M. Zachwieja, R. W. Field, Wojciech Szajna, Małgorzata Ostrowska-Kopeć, Edcel J. Salumbides, Przemysław Kolek
Publikováno v:
RSC Adv.
High-accuracy dispersive optical spectroscopy measurements in the visible (VIS) region have been performed on the less-abundant 12C17O isotopologue, observing high-resolution emission bands of the B1Σ+ (υ = 0) → A1Π (υ = 3, 4, and 5) Angstrom s
Publikováno v:
The Astrophysical Journal. 902:141
The prevalence of substructures in $\sim1-10$ Myr old protoplanetary disks, which are often linked to planet formation, has raised the question of how early such features form, and as a corollary, how early planet formation begins. Here we present ob
Publikováno v:
Proceedings of the International Astronomical Union. 11:282-286
Laboratory astrophysics is the Rosetta stone that enables astronomers to understand and interpret the cosmos. The IAU Commission 14, the predecessor of the new IAU Laboratory Astrophysics Commission C. B5 and the AAS Laboratory Astrophysics Division