ScholarGate
Trợ lý

So sánh phương pháp

Xem các phương pháp đã chọn cạnh nhau; những hàng khác biệt được làm nổi bật.

Khoảng cách Động học×Mảng thời gian pulsar×Phân tích đường cong quay×
Lĩnh vựcThiên văn họcThiên văn họcThiên văn học
HọProcess / pipelineProcess / pipelineProcess / pipeline
Năm ra đời195719791970
Người khởi xướngBert WesterhoutStephen DetweilerVera Rubin
LoạiKinematic measurement methodObservational timing methodObservational kinematic method
Công trình gốcReid, M. J., et al. (2014). Trigonometric parallaxes of high mass star forming regions: the structure and kinematics of the Milky Way. Astrophysical Journal, 783(2), 130. DOI ↗Sazhin, M. V. (1978). Opportunities for detecting ultralong gravitational waves. Soviet Astronomy, 22, 36-38. link ↗Vera C. Rubin & W. Kent Ford Jr. (1970). Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission Regions. Astrophysical Journal, 159, 379-403. DOI ↗
Tên gọi khácGalactic Kinematic Distances, Rotation-Curve Distance, Kinematic ParallaxPTA, Millisecond Pulsar Timing, Pulsar Timing ResidualsGalactic Rotation Curves, Rotation Curve Method, Velocity Curve Analysis
Liên quan333
Tóm tắtKinematic distance is a method for estimating distances to objects in the Milky Way using their observed radial velocities and the known rotation curve of the Galaxy. Developed in the 1950s by Bert Westerhout and others, this technique enables distance determination to distant molecular clouds and masers without trigonometric parallax or individual object luminosities.A pulsar timing array uses multiple millisecond pulsars as a distributed network of gravitational wave detectors across the galaxy. Proposed theoretically by Stephen Detweiler in 1979, this method exploits the extraordinary timing precision of pulsars to detect the subtle spacetime distortions caused by gravitational waves. In 2023, the first evidence for a stochastic background of gravitational waves was announced using pulsar timing arrays.Galaxy rotation curve analysis is the technique of measuring how orbital velocities change with distance from the center of a galaxy. Pioneered by Vera Rubin and W. Kent Ford Jr. in 1970, rotation curves revealed one of astronomy's great mysteries: galaxies rotate too fast to be held together by their visible stars alone, providing direct evidence for dark matter.
ScholarGateBộ dữ liệu
  1. v1
  2. 3 Nguồn tài liệu
  3. PUBLISHED
  1. v1
  2. 3 Nguồn tài liệu
  3. PUBLISHED
  1. v1
  2. 3 Nguồn tài liệu
  3. PUBLISHED

Đến trang tìm kiếm Tải xuống bản trình chiếu

ScholarGateSo sánh phương pháp: Kinematic Distance · Pulsar Timing Array · Rotation Curve Analysis. Truy cập ngày 2026-06-19 từ https://scholargate.app/vi/compare