IRAS 22130+5634 , the SIMBAD biblio

IRAS 22130+5634 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST01:28:42


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Title First 3 Authors
1988IRASP.C......0J viz 14       D               1 245223 ~ Infrared Astronomical Satellite Catalogs, 1988. The Point Source Catalog, version 2.0, NASA RP-1190 JOINT IRAS SCIENCE WORKING GROUP
1991AJ....102..289B 105 38 The mass range of carbon stars. BARNBAUM C., KASTNER J.H. and ZUCKERMAN B.
1993A&A...267...39B 52 42 Candidate OH/IR stars in the outer parts of our galaxy. BLOMMAERT J.A.D.L., VAN DER VEEN W.E.C.J. and HABING H.J.
1993A&A...275..163K viz 64 45 Probing the AGB tip : luminous carbon stars in the galactic plane. KASTNER J.H., FORVEILLE T., ZUCKERMAN B., et al.
1993A&AS...98..589W viz 1214 138 IRAS sources beyond the solar circle. III. Observations of H2O, OH, CH3OH and CO. WOUTERLOOT J.G.A., BRAND J. and FIEGLE K.
1993A&AS...99..291L viz 451 464 CO and HCN observations of circumstellar envelopes. A catalogue - mass loss rates and distributions. LOUP C., FORVEILLE T., OMONT A., et al.
1996AJ....111..231J 103 9 Optical identification of IRAS sources in the outer galaxy. JIANG B.W., DEGUCHI S. and NAKADA Y.
1996ApJS..106..463J viz 182 42 SiO maser sources in the outer disk of the galaxy. JIANG B.W., DEGUCHI S., YAMAMURA I., et al.
1997AJ....113.1315J 95 21 Identification of IRAS sources in the outer disk of the galaxy. JIANG B.W., DEGUCHI S., HU J.Y., et al.
1997ApJS..112..557K viz 11276 205 Classification and identification of IRAS sources with low-resolution spectra. KWOK S., VOLK K. and BIDELMAN W.P.
2003A&A...399.1083K viz 6713 27 The association of IRAS sources and 12CO emission in the outer Galaxy. KERTON C.R. and BRUNT C.M.
2006A&A...445.1069G 268 83 Infrared photometry and evolution of mass-losing AGB stars. I. Carbon stars revisited. GUANDALINI R., BUSSO M., CIPRINI S., et al.
2012AJ....144...10C 130       D     X         4 87 0 Newly identified carbon stars from sources with unusual IRAS low-resolution spectra. CHEN P.S. and SHAN H.G.

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