Energy distribution in giants and supergiants.

Dataset

The energy distributions for 27 giants and supergiants of the M spectral type are presented in the region of 3200-7600{AA} with the step of 50{AA}. The observations were made in the Fessenkov Astrophysical institute (Alma-Ata) during 1986-1987 with a spectrophotometer of Seya-Namioka mounted on the 50-cm Cassegrain telescope. The primary standard is Vega with the energy distribution by Hayes (1985IAUS..111..225H). The relative r.m.s. of the results are given in the table3.dat.

Cone search capability for table J/AZh/73/762/table2 (Information about the stars)

Identifier
Source	https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AZh/73/762
Related Identifier	https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/73/762
Related Identifier	http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AZh/73/762
Metadata Access	http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AZh/73/762

Provenance
Creator	Tereshchenko V.M.
Publisher	CDS
Publication Year	1998
Rights	https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess	true
Contact	CDS support team <cds-question(at)unistra.fr>

Representation
Resource Type	Dataset; AstroObjects
Discipline	Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy