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International Astronomical Union Colloquium
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International Astronomical Union Colloquium
Article . 1983 . Peer-reviewed
License: Cambridge Core User Agreement
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https://doi.org/10.1007/978-94...
Part of book or chapter of book . 1983 . Peer-reviewed
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Optical Monitoring of T Tauri Stars

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Other literature type 01 Jan 1983Publisher:Springer NetherlandsJournal:International Astronomical Union Colloquium, volume 71, pages 501-502 (issn: 0252-9211, Copyright policy )
Authors: William Herbst;

doi: 10.1007/978-94-009-7157-8_70 , 10.1017/s0252921100096573

Optical Monitoring of T Tauri Stars

Abstract

At the Van Vleck Observatory of Wesleyan University, Middletown, Connecticut, we have initiated a program of monitoring T Tauri stars with the 24-inch reflector (Perkin Telescope). During the first observing season, we have obtained UBVRI and Hα (30Å and 150Å) data for five stars: T Tau, RY Tau, SU Aur, RW Aur, and CO Ori. The data will be presented elsewhere (Herbst, Holtzman and Phelps, 1982). Here we re-port some of our conclusions.

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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