The force exerted by the stellar system in the direction perpendicular to the galactic plane and some related problems

By J. Oort. 1932

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

1. M. Cappellari
2. S. Courteau
3. P. Hopkins
4. A. Dutton
5. T. Treu
6. Eric Emsellem
7. C. Conroy
8. S. McGaugh

Citations in the corpus

• The Phenomenology of Right Handed Neutrinos (2013, result): “In contrast to that, HDM predicts that large structures form first [299] because primordial fluctuations in the gravitational potential have been erased due to the large free streaming length (63)The term “dark matter” was already used in [481, 482], but in that context simply referred to non-lumino”
• General Relativity and Cosmology: Unsolved Questions and Future Directions (2016, background): “Radio astronomy pioneer Jan Oort also hypothesized the existence of Dark Matter in 1932 [228].”
• A review of indirect searches for particle dark matter (2016, methodology): “Earlier suggestions of missing mass from observations of the Milky Way were made by Kapteyn in 1922, also at Mount Wilson Observatory [2], and by Oort in 1932 at Leiden Observatory [3].”
• WIMP dark matter candidates and searches—current status and future prospects (2017, background): “ in the case of strong lensing, or when light travels far from the core of the galaxy or cluster, the eect is much weaker. However, it can still 2Earlier speculations were made by Kapteyn [14], Oort [15] and Jeans [16]. For a historical development, see [17]. { 3 { (a) (b) Figure 1: (a) Strong gravi”
• Effect of Sun and Planet-Bound Dark Matter on Planet and Satellite Dynamics in the Solar System (2010, background): “Oort concluded that the total mass of nebulous or meteoric matter near the Sun is less than 3 × 10−24 g cm−3.”
• Optimized dark matter searches in deep observations of Segue 1 with MAGIC (2013, background): “Although works of Öpik (1922) [1] and of Oort (1932) [2] were implying that the luminous components of the galaxies were not sufficiently massive to explain their dynamics, it was Zwicky that first adopted the concept of dark matter in 1933 [3].”
• Dark Matter: A Primer (2010, background): “However, Oort noted that another possible explanation was that 85% of the light from the galactic center was obscured by dust and intervening matter or that the velocity measurements for the stars in question were simply in error [1].”
• Mirror particles and mirror matter: 50 years of speculation and searching (2006, background): “ [200, 201] was questioned [205, 206] (see the discussion [207, 208]), many astrophysicists believe that the stellar dark matter cannot consist of ordinary baryons [209, 210]. Since the times of Oort [40] and Zwicky [41, 42] there existed two alternative explanations of anomalously high velocities o”
• Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions (2011, background): “Oort [342] noted that the sum of the observed stars in the vicinity of the sun fell short of explaining the vertical motions of stars in the disk of the Milky Way.”
• Dark Matter (2011, unknown): “The dark matter problem was discussed in a regional conference on January 1975 in Tallinn.”
• Galaxy Masses: A Review (2013, methodology): “The first detailed analysis of this type was carried out by Oort (1932) who built upon earlier and important work by Kapteyn (1922) and Jeans (1922).”