Đường cong quay thiên hà (Vietnamese Wikipedia)

Analysis of information sources in references of the Wikipedia article "Đường cong quay thiên hà" in Vietnamese language version.

refsWebsite

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archive.org (Global: 6^th place; Vietnamese: 4^th place)

Corbelli, E.; Salucci, P. (2000). "The extended rotation curve and the dark matter halo of M33". Monthly Notices of the Royal Astronomical Society. Quyển 311 số 2. tr. 441–447. arXiv:astro-ph/9909252. Bibcode:2000MNRAS.311..441C. doi:10.1046/j.1365-8711.2000.03075.x.
The explanation of the mass discrepancy in spiral galaxies by means of massive and extensive dark component was first put forward by A. Bosma in a PhD dissertation, see
Bosma, A. (1978). The Distribution and Kinematics of Neutral Hydrogen in Spiral Galaxies of Various Morphological Types (PhD). Rijksuniversiteit Groningen. Truy cập ngày 30 tháng 12 năm 2016 – qua NASA/IPAC Extragalactic Database.See also

Rubin, V.; Thonnard, N.; Ford, W. K. Jr. (1980). "Rotational Properties of 21 Sc Galaxies With a Large Range of Luminosities and Radii from NGC 4605 (R=4kpc) to UGC 2885 (R=122kpc)". The Astrophysical Journal. Quyển 238. tr. 471–487. Bibcode:1980ApJ...238..471R. doi:10.1086/158003.

Begeman, K. G.; Broeils, A. H.; Sanders, R.H. (1991). "Extended Rotation Curves of Spiral Galaxies: Dark Haloes and Modified Dynamics". Monthly Notices of the Royal Astronomical Society. Quyển 249 số 3. tr. 523–537. Bibcode:1991MNRAS.249..523B. doi:10.1093/mnras/249.3.523.

arxiv.org (Global: 69^th place; Vietnamese: 100^th place)

Corbelli, E.; Salucci, P. (2000). "The extended rotation curve and the dark matter halo of M33". Monthly Notices of the Royal Astronomical Society. Quyển 311 số 2. tr. 441–447. arXiv:astro-ph/9909252. Bibcode:2000MNRAS.311..441C. doi:10.1046/j.1365-8711.2000.03075.x.
For an extensive discussion of the data and its fit to MOND see Milgrom, M. (2007). "The MOND Paradigm". arXiv:0801.3133 [astro-ph].

caltech.edu (Global: 887^th place; Vietnamese: 588^th place)

nedipac.caltech.edu

The explanation of the mass discrepancy in spiral galaxies by means of massive and extensive dark component was first put forward by A. Bosma in a PhD dissertation, see
Bosma, A. (1978). The Distribution and Kinematics of Neutral Hydrogen in Spiral Galaxies of Various Morphological Types (PhD). Rijksuniversiteit Groningen. Truy cập ngày 30 tháng 12 năm 2016 – qua NASA/IPAC Extragalactic Database.See also

Rubin, V.; Thonnard, N.; Ford, W. K. Jr. (1980). "Rotational Properties of 21 Sc Galaxies With a Large Range of Luminosities and Radii from NGC 4605 (R=4kpc) to UGC 2885 (R=122kpc)". The Astrophysical Journal. Quyển 238. tr. 471–487. Bibcode:1980ApJ...238..471R. doi:10.1086/158003.

Begeman, K. G.; Broeils, A. H.; Sanders, R.H. (1991). "Extended Rotation Curves of Spiral Galaxies: Dark Haloes and Modified Dynamics". Monthly Notices of the Royal Astronomical Society. Quyển 249 số 3. tr. 523–537. Bibcode:1991MNRAS.249..523B. doi:10.1093/mnras/249.3.523.
Bosma, A. (1978). The Distribution and Kinematics of Neutral Hydrogen in Spiral Galaxies of Various Morphological Types (PhD). Rijksuniversiteit Groningen. Truy cập ngày 30 tháng 12 năm 2016 – qua NASA/IPAC Extragalactic Database.

doi.org (Global: 2^nd place; Vietnamese: 2^nd place)

Corbelli, E.; Salucci, P. (2000). "The extended rotation curve and the dark matter halo of M33". Monthly Notices of the Royal Astronomical Society. Quyển 311 số 2. tr. 441–447. arXiv:astro-ph/9909252. Bibcode:2000MNRAS.311..441C. doi:10.1046/j.1365-8711.2000.03075.x.
The explanation of the mass discrepancy in spiral galaxies by means of massive and extensive dark component was first put forward by A. Bosma in a PhD dissertation, see
Bosma, A. (1978). The Distribution and Kinematics of Neutral Hydrogen in Spiral Galaxies of Various Morphological Types (PhD). Rijksuniversiteit Groningen. Truy cập ngày 30 tháng 12 năm 2016 – qua NASA/IPAC Extragalactic Database.See also

Rubin, V.; Thonnard, N.; Ford, W. K. Jr. (1980). "Rotational Properties of 21 Sc Galaxies With a Large Range of Luminosities and Radii from NGC 4605 (R=4kpc) to UGC 2885 (R=122kpc)". The Astrophysical Journal. Quyển 238. tr. 471–487. Bibcode:1980ApJ...238..471R. doi:10.1086/158003.

Begeman, K. G.; Broeils, A. H.; Sanders, R.H. (1991). "Extended Rotation Curves of Spiral Galaxies: Dark Haloes and Modified Dynamics". Monthly Notices of the Royal Astronomical Society. Quyển 249 số 3. tr. 523–537. Bibcode:1991MNRAS.249..523B. doi:10.1093/mnras/249.3.523.

harvard.edu (Global: 18^th place; Vietnamese: 24^th place)

ui.adsabs.harvard.edu

Corbelli, E.; Salucci, P. (2000). "The extended rotation curve and the dark matter halo of M33". Monthly Notices of the Royal Astronomical Society. Quyển 311 số 2. tr. 441–447. arXiv:astro-ph/9909252. Bibcode:2000MNRAS.311..441C. doi:10.1046/j.1365-8711.2000.03075.x.
The explanation of the mass discrepancy in spiral galaxies by means of massive and extensive dark component was first put forward by A. Bosma in a PhD dissertation, see
Bosma, A. (1978). The Distribution and Kinematics of Neutral Hydrogen in Spiral Galaxies of Various Morphological Types (PhD). Rijksuniversiteit Groningen. Truy cập ngày 30 tháng 12 năm 2016 – qua NASA/IPAC Extragalactic Database.See also

Rubin, V.; Thonnard, N.; Ford, W. K. Jr. (1980). "Rotational Properties of 21 Sc Galaxies With a Large Range of Luminosities and Radii from NGC 4605 (R=4kpc) to UGC 2885 (R=122kpc)". The Astrophysical Journal. Quyển 238. tr. 471–487. Bibcode:1980ApJ...238..471R. doi:10.1086/158003.

Begeman, K. G.; Broeils, A. H.; Sanders, R.H. (1991). "Extended Rotation Curves of Spiral Galaxies: Dark Haloes and Modified Dynamics". Monthly Notices of the Royal Astronomical Society. Quyển 249 số 3. tr. 523–537. Bibcode:1991MNRAS.249..523B. doi:10.1093/mnras/249.3.523.