The Variability of T Tauri, RY Tauri, and RW Aurigae from 1899 to 1952-Reference-Cited by-同舟云学术

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The Variability of T Tauri, RY Tauri, and RW Aurigae from 1899 to 1952

Published:2001-07 Issue:1 Volume:122 Page:413-417
ISSN:0004-6256
Container-title:The Astronomical Journal
language:
Short-container-title:

Author:

Beck Tracy L.,Simon M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/1538-3881/122/i=1/a=413/pdf

Reference42 articles.

1. A Circumstellar Dust Disk around T Tauri N: Subarcsecond Imaging at λ = 3 Millimeters

2. Ambartsumian, V. A. 1947, Stellar Evolution and Astrophysics (Yerevan: Acad. Sci. Armenian SSR)

3. Hamilton echelle spectra of young stars. I - Optical veiling

4. Beck, T. L. 2001, Ph.D. thesis, SUNY Stony Brook, in preparation

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2. Time-variable Jet Ejections from RW Aur A, RY Tau, and DG Tau*;The Astrophysical Journal Supplement Series;2022-12-13

3. Optical and Near-infrared Excesses are Correlated in T Tauri Stars;The Astrophysical Journal;2022-04-01

4. On the Nature of the T Tauri Triple System;The Astrophysical Journal;2020-10-21

5. Possible Time Correlation between Jet Ejection and Mass Accretion for RW Aur A;The Astrophysical Journal;2020-09-17

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