Near-infrared variability (1-10) microns of Herbig-Haro exciting sources

Details Near-infrared variability (1-10) microns of Herbig-Haro exciting sources Near-infrared variability (1-10) microns of Herbig-Haro exciting sources

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ncimc..15.1033m&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 15 C, no. 6, p. 1033-1038.

Astronomy and Astrophysics

Astronomy

1

Accretion Disks, Herbig-Haro Objects, Infrared Sources (Astronomy), Stellar Spectra, Astronomical Spectroscopy, Infrared Astronomy, Stellar Winds

Scientific paper

First results of observations of photometric variations in the near infrared are presented for the young and active low-luminosity objects NGC 1333 IRS 13 and L 1551 IRS 5. Based on the results of a preliminary analysis, it is suggested that accretion phenomena occurring in the disks should be considered among other plausible causes for the observed near-IR variations.

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