Арки (скупчення) (Ukrainian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Арки (скупчення)" in Ukrainian language version.

refsWebsite

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7arxiv.org

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7harvard.edu

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7doi.org

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2worldcat.org

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1newscientist.com

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1web.archive.org

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archive.org

Blum, R. D.; Schaerer, D.; Pasquali, A.; Heydari-Malayeri, M.; Conti, P. S.; Schmutz, W. (2001). 2 Micron Narrowband Adaptive Optics Imaging in the Arches Cluster. The Astronomical Journal. 122 (4): 1875. arXiv:astro-ph/0106496. Bibcode:2001AJ....122.1875B. doi:10.1086/323096.

arxiv.org

Espinoza, P.; Selman3, F. J.; Melnick, J. (July 2009). The massive star initial mass function of the Arches cluster. Astronomy and Astrophysics. 504 (2): 563—583. arXiv:0903.2222. Bibcode:2009A&A...501..563E. doi:10.1051/0004-6361/20078597. {{cite journal}}: |access-date= вимагає |url= (довідка)
Figer, Donald F. (2005). An upper limit to the masses of stars. Nature. 434 (7030): 192—194. arXiv:astro-ph/0503193. Bibcode:2005Natur.434..192F. doi:10.1038/nature03293. ISSN 0028-0836.
Habibi, M.; Stolte, A.; Brandner, W.; Hußmann, B.; Motohara, K. (August 2013). The Arches cluster out to its tidal radius: dynamical mass segregation and the effect of the extinction law on the stellar mass function. Astronomy and Astrophysics. 556 (A26). arXiv:1212.3355. Bibcode:2013A&A...556A..26H. doi:10.1051/0004-6361/201220556. {{cite journal}}: |access-date= вимагає |url= (довідка)
Blum, R. D.; Schaerer, D.; Pasquali, A.; Heydari-Malayeri, M.; Conti, P. S.; Schmutz, W. (2001). 2 Micron Narrowband Adaptive Optics Imaging in the Arches Cluster. The Astronomical Journal. 122 (4): 1875. arXiv:astro-ph/0106496. Bibcode:2001AJ....122.1875B. doi:10.1086/323096.
Figer, D. F.; Najarro, F.; Gilmore, D.; Morris, M.; Kim, S. S.; Serabyn, E.; McLean, I. S.; Gilbert, A. M.; Graham, J. R.; Larkin, J. E.; Levenson, N. A.; Teplitz, H. I. (2002). Massive Stars in the Arches Cluster. The Astrophysical Journal. 581: 258. arXiv:astro-ph/0208145. Bibcode:2002ApJ...581..258F. doi:10.1086/344154.
Martins, F.; Hillier, D. J.; Paumard, T.; Eisenhauer, F.; Ott, T.; Genzel, R. (2008). The most massive stars in the Arches cluster. Astronomy and Astrophysics. 478: 219. arXiv:0711.0657. Bibcode:2008A&A...478..219M. doi:10.1051/0004-6361:20078469.
Gräfener, G.; Vink, J. S.; de Koter, A.; Langer, N. (2011). The Eddington factor as the key to understand the winds of the most massive stars. Astronomy & Astrophysics. 535: A56. arXiv:1106.5361. Bibcode:2011A&A...535A..56G. doi:10.1051/0004-6361/201116701. ISSN 0004-6361.

doi.org

Espinoza, P.; Selman3, F. J.; Melnick, J. (July 2009). The massive star initial mass function of the Arches cluster. Astronomy and Astrophysics. 504 (2): 563—583. arXiv:0903.2222. Bibcode:2009A&A...501..563E. doi:10.1051/0004-6361/20078597. {{cite journal}}: |access-date= вимагає |url= (довідка)
Figer, Donald F. (2005). An upper limit to the masses of stars. Nature. 434 (7030): 192—194. arXiv:astro-ph/0503193. Bibcode:2005Natur.434..192F. doi:10.1038/nature03293. ISSN 0028-0836.
Habibi, M.; Stolte, A.; Brandner, W.; Hußmann, B.; Motohara, K. (August 2013). The Arches cluster out to its tidal radius: dynamical mass segregation and the effect of the extinction law on the stellar mass function. Astronomy and Astrophysics. 556 (A26). arXiv:1212.3355. Bibcode:2013A&A...556A..26H. doi:10.1051/0004-6361/201220556. {{cite journal}}: |access-date= вимагає |url= (довідка)
Blum, R. D.; Schaerer, D.; Pasquali, A.; Heydari-Malayeri, M.; Conti, P. S.; Schmutz, W. (2001). 2 Micron Narrowband Adaptive Optics Imaging in the Arches Cluster. The Astronomical Journal. 122 (4): 1875. arXiv:astro-ph/0106496. Bibcode:2001AJ....122.1875B. doi:10.1086/323096.
Figer, D. F.; Najarro, F.; Gilmore, D.; Morris, M.; Kim, S. S.; Serabyn, E.; McLean, I. S.; Gilbert, A. M.; Graham, J. R.; Larkin, J. E.; Levenson, N. A.; Teplitz, H. I. (2002). Massive Stars in the Arches Cluster. The Astrophysical Journal. 581: 258. arXiv:astro-ph/0208145. Bibcode:2002ApJ...581..258F. doi:10.1086/344154.
Martins, F.; Hillier, D. J.; Paumard, T.; Eisenhauer, F.; Ott, T.; Genzel, R. (2008). The most massive stars in the Arches cluster. Astronomy and Astrophysics. 478: 219. arXiv:0711.0657. Bibcode:2008A&A...478..219M. doi:10.1051/0004-6361:20078469.
Gräfener, G.; Vink, J. S.; de Koter, A.; Langer, N. (2011). The Eddington factor as the key to understand the winds of the most massive stars. Astronomy & Astrophysics. 535: A56. arXiv:1106.5361. Bibcode:2011A&A...535A..56G. doi:10.1051/0004-6361/201116701. ISSN 0004-6361.

harvard.edu

ui.adsabs.harvard.edu

Espinoza, P.; Selman3, F. J.; Melnick, J. (July 2009). The massive star initial mass function of the Arches cluster. Astronomy and Astrophysics. 504 (2): 563—583. arXiv:0903.2222. Bibcode:2009A&A...501..563E. doi:10.1051/0004-6361/20078597. {{cite journal}}: |access-date= вимагає |url= (довідка)
Figer, Donald F. (2005). An upper limit to the masses of stars. Nature. 434 (7030): 192—194. arXiv:astro-ph/0503193. Bibcode:2005Natur.434..192F. doi:10.1038/nature03293. ISSN 0028-0836.
Habibi, M.; Stolte, A.; Brandner, W.; Hußmann, B.; Motohara, K. (August 2013). The Arches cluster out to its tidal radius: dynamical mass segregation and the effect of the extinction law on the stellar mass function. Astronomy and Astrophysics. 556 (A26). arXiv:1212.3355. Bibcode:2013A&A...556A..26H. doi:10.1051/0004-6361/201220556. {{cite journal}}: |access-date= вимагає |url= (довідка)
Blum, R. D.; Schaerer, D.; Pasquali, A.; Heydari-Malayeri, M.; Conti, P. S.; Schmutz, W. (2001). 2 Micron Narrowband Adaptive Optics Imaging in the Arches Cluster. The Astronomical Journal. 122 (4): 1875. arXiv:astro-ph/0106496. Bibcode:2001AJ....122.1875B. doi:10.1086/323096.
Figer, D. F.; Najarro, F.; Gilmore, D.; Morris, M.; Kim, S. S.; Serabyn, E.; McLean, I. S.; Gilbert, A. M.; Graham, J. R.; Larkin, J. E.; Levenson, N. A.; Teplitz, H. I. (2002). Massive Stars in the Arches Cluster. The Astrophysical Journal. 581: 258. arXiv:astro-ph/0208145. Bibcode:2002ApJ...581..258F. doi:10.1086/344154.
Martins, F.; Hillier, D. J.; Paumard, T.; Eisenhauer, F.; Ott, T.; Genzel, R. (2008). The most massive stars in the Arches cluster. Astronomy and Astrophysics. 478: 219. arXiv:0711.0657. Bibcode:2008A&A...478..219M. doi:10.1051/0004-6361:20078469.
Gräfener, G.; Vink, J. S.; de Koter, A.; Langer, N. (2011). The Eddington factor as the key to understand the winds of the most massive stars. Astronomy & Astrophysics. 535: A56. arXiv:1106.5361. Bibcode:2011A&A...535A..56G. doi:10.1051/0004-6361/201116701. ISSN 0004-6361.

newscientist.com

space.newscientist.com

Про швидкість на сайті VLT. [Архівовано 6 липня 2008 у Wayback Machine.] (англ.)

web.archive.org

Про швидкість на сайті VLT. [Архівовано 6 липня 2008 у Wayback Machine.] (англ.)

worldcat.org

Figer, Donald F. (2005). An upper limit to the masses of stars. Nature. 434 (7030): 192—194. arXiv:astro-ph/0503193. Bibcode:2005Natur.434..192F. doi:10.1038/nature03293. ISSN 0028-0836.
Gräfener, G.; Vink, J. S.; de Koter, A.; Langer, N. (2011). The Eddington factor as the key to understand the winds of the most massive stars. Astronomy & Astrophysics. 535: A56. arXiv:1106.5361. Bibcode:2011A&A...535A..56G. doi:10.1051/0004-6361/201116701. ISSN 0004-6361.