1-4 μm spectroscopy of very red stars found in an I-band objective prism survey

Miwa Goto; Yoshinori Sasaki; Masatoshi Imanishi; Tetsuya Nagata; Terry Jay Jones

doi:10.1093/pasj/49.4.485

1-4 μm spectroscopy of very red stars found in an I-band objective prism survey

Miwa Goto, Yoshinori Sasaki, Masatoshi Imanishi, Tetsuya Nagata, Terry Jay Jones

Minnesota Institute for Astrophysics

Research output: Contribution to journal › Article › peer-review

6 Scopus citations

Abstract

We present the 1.2-4.2 μm spectroscopy of stars found in an objective prism survey of the galactic plane by Stephenson (1992, AAA 55.002.010). These stars were thought by Stephenson to be heavily reddened by interstellar absorption. However, almost all of them have turned out to be late-type stars with clear 2.3 μm CO absorption, which means that they are intrinsically red as well. A few stars have A_V ∼ 9, but most of them are only moderately reddened (A_V = 1-5).

Original language	English (US)
Pages (from-to)	485-492
Number of pages	8
Journal	Publications of the Astronomical Society of Japan
Volume	49
Issue number	4
DOIs	https://doi.org/10.1093/pasj/49.4.485
State	Published - 1997

Keywords

Infrared: spectra
Interstellar: extinction
Stars: classification
Stars: late-type

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abstract = "We present the 1.2-4.2 μm spectroscopy of stars found in an objective prism survey of the galactic plane by Stephenson (1992, AAA 55.002.010). These stars were thought by Stephenson to be heavily reddened by interstellar absorption. However, almost all of them have turned out to be late-type stars with clear 2.3 μm CO absorption, which means that they are intrinsically red as well. A few stars have AV ∼ 9, but most of them are only moderately reddened (AV = 1-5).",

keywords = "Infrared: spectra, Interstellar: extinction, Stars: classification, Stars: late-type",

author = "Miwa Goto and Yoshinori Sasaki and Masatoshi Imanishi and Tetsuya Nagata and Jones, {Terry Jay}",

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doi = "10.1093/pasj/49.4.485",

language = "English (US)",

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T1 - 1-4 μm spectroscopy of very red stars found in an I-band objective prism survey

AU - Goto, Miwa

AU - Sasaki, Yoshinori

AU - Imanishi, Masatoshi

AU - Nagata, Tetsuya

AU - Jones, Terry Jay

PY - 1997

Y1 - 1997

N2 - We present the 1.2-4.2 μm spectroscopy of stars found in an objective prism survey of the galactic plane by Stephenson (1992, AAA 55.002.010). These stars were thought by Stephenson to be heavily reddened by interstellar absorption. However, almost all of them have turned out to be late-type stars with clear 2.3 μm CO absorption, which means that they are intrinsically red as well. A few stars have AV ∼ 9, but most of them are only moderately reddened (AV = 1-5).

AB - We present the 1.2-4.2 μm spectroscopy of stars found in an objective prism survey of the galactic plane by Stephenson (1992, AAA 55.002.010). These stars were thought by Stephenson to be heavily reddened by interstellar absorption. However, almost all of them have turned out to be late-type stars with clear 2.3 μm CO absorption, which means that they are intrinsically red as well. A few stars have AV ∼ 9, but most of them are only moderately reddened (AV = 1-5).

KW - Infrared: spectra

KW - Interstellar: extinction

KW - Stars: classification

KW - Stars: late-type

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DO - 10.1093/pasj/49.4.485

M3 - Article

AN - SCOPUS:0031286750

VL - 49

SP - 485

EP - 492

JO - Publication of the Astronomical Society of Japan

JF - Publication of the Astronomical Society of Japan

SN - 0004-6264

IS - 4

ER -

1-4 μm spectroscopy of very red stars found in an I-band objective prism survey

Abstract

Keywords

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