Zobrazeno 1 - 10
of 242
pro vyhledávání: '"Perseus Arm"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 509:68-84
Expansion of (sub)millimetre capabilities to high angular resolution offered with interferometers allows to resolve giant molecular clouds (GMCs) in nearby galaxies. This enables us to place the Milky Way in the context of other galaxies to advance o
Autor:
E. E. Lekht, G. M. Rudnitskii, M. I. Pashchenko, N. T. Ashimbaeva, V. V. Krasnov, A. M. Tolmachev, P. Colom
Publikováno v:
Astronomy Reports. 64:839-854
We present the results of our observations of the star-forming region located in the Perseus arm and associated with the Sharpless nebula S231 in the lines of H2O at a wavelength of 1.35 cm and OH at a wavelength of 18 cm obtained with the Pushchino
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 487:2771-2784
The Perseus Arm is the closest Galactic spiral arm from the Sun, offering an excellent opportunity to study in detail its stellar population. However, its distance has been controversial with discrepancies by a factor of two. Kinematic distances are
Autor:
Alan Jackson, Steven J. Desch
Publikováno v:
Journal of Geophysical Research: Planets. 126
The origin of the interstellar object 1I/'Oumuamua has defied explanation. We perform calculations of the non-gravitational acceleration that would be experienced by bodies composed of a range of different ices and demonstrate that a body composed of
Autor:
Steven J. Desch, Alan Jackson
The origin of the interstellar object 1I/'Oumuamua, has defied explanation. In a companion paper (Jackson & Desch, 2021), we show that a body of N2 ice with axes 45 m x 44 m x 7.5 m at the time of observation would be consistent with its albedo, non-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4ebb6c4d0cc5ba3dd85627dd0465f84f
http://arxiv.org/abs/2103.08812
http://arxiv.org/abs/2103.08812
Autor:
Morgan Fouesneau, D. J. Marshall, Rene Andrae, Vincenzo Ripepi, Ronald Drimmel, Yves Fremat, P. Ramos, Gisella Clementini, Alex Lobel, Tristan Cantat-Gaudin, M. Romero-Gómez, Laurent Chemin, E. Poggio, T. Muraveva, R. Blomme, E. Zari, F. Figueras
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 651, pp.A104. ⟨10.1051/0004-6361/202140687⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2021, 651, pp.A104. ⟨10.1051/0004-6361/202140687⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 651, pp.A104. ⟨10.1051/0004-6361/202140687⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2021, 651, pp.A104. ⟨10.1051/0004-6361/202140687⟩
Using the astrometry and integrated photometry from the Gaia Early Data Release 3 (EDR3), we map the density variations in the distribution of young Upper Main Sequence (UMS) stars, open clusters and classical Cepheids in the Galactic disk within sev
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a73bc53fa02879f61b44da8a52cd63be
http://arxiv.org/abs/2103.01970
http://arxiv.org/abs/2103.01970
We cross-match the Alma catalog of OB stars with Gaia DR2 astrometry and photometry as a first step towards producing a clean sample of massive stars in the solar neighbourhood with a high degree of completeness. We analyze the resulting colour-absol
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a32ce638bbbdccd987981f00b74ed133
Autor:
Márcio Catelan, Vittorio F. Braga, R. Contreras Ramos, Marcella Marconi, Sonia Duffau, Dante Minniti, A. A. R. Valcarce, Wolfgang Gieren, Luca Sbordone, J. H. Minniti, Manuela Zoccali, A. Rojas-Arriagada
In an effort to improve our understanding of the spiral arm structure of the Milky Way, we use Classical Cepheids (CCs) to increase the number of young tracers on the far side of the Galactic disk with accurately determined distances. We use a sample
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4473985b5da8e0639291be596e3a139d
http://hdl.handle.net/20.500.12386/31902
http://hdl.handle.net/20.500.12386/31902
Autor:
A. K. Mainzer, Tony Travouillon, Anna M. Moore, Michael C. B. Ashley, Matthew J. Hankins, Ryan M. Lau, Viraj Karambelkar, Roc M. Cutri, Luisa Rebull, Kaushik De, Lynne A. Hillenbrand, Mansi M. Kasliwal
We report the discovery of a likely outbursting Class I young stellar object, associated with the star-forming region NGC 281-W (distance $\sim 2.8$ kpc). The source is currently seen only at infrared wavelengths, appearing in both the Palomar Gattin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dbf935ff7e095347cdf8b17dc7faf129
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Universidade de São Paulo (USP)
instacron:USP
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the origina
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f8c87261ab26131fda37181f2ad28cf8