IRAS 19261+1435 , the SIMBAD biblio

IRAS 19261+1435 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST15:55:19

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1988ApJS...66..183E 178 134 New OH/IR stars from color-selected iras sources : 1612 MHz observations. EDER J., LEWIS B.M. and TERZIAN Y.
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
1991A&AS...90..327T viz 2734 208 1612 MHz OH survey of IRAS point sources. I. Observations made at Dwingeloo, Effelsberg and Parkes. TE LINTEL HEKKERT P., CASWELL J.L., HABING H.J., et al.
1996A&AS..116..117E 389 52 A survey for 22GHz water maser emission from the Arecibo set of OH/IR stars. ENGELS D. and LEWIS B.M.
1997ApJS..109..489L viz 394 20 Main-line OH observations of the Arecibo set of OH/IR stars. LEWIS B.M.
2004AJ....127..501L viz 135 9 2MASS counterparts for OH/IR stars. I. The Arecibo sample. LEWIS B.M., KOPON D.A. and TERZIAN Y.
2005A&A...431..779J viz 376 18 An infrared study of galactic OH/IR stars. I. An optical/near-IR atlas of the Arecibo sample. JIMENEZ-ESTEBAN F.M., AGUDO-MERIDA L., ENGELS D., et al.
2017ApJS..232...13C 16       D               2 254 2 Simultaneous observations of H2O and SiO masers toward OH/IR stars. CHO C.-Y., CHO S.-H., KIM S., et al.
2020ApJ...891...50U 16       D               1 116 ~ The 3D distribution of Long-period Mira variables in the Galactic disk. URAGO R., OMODAKA T., NAGAYAMA T., et al.
2021MNRAS.505.6051J viz 17       D               2 392 1 An infrared study of Galactic OH/IR stars - III. Variability properties of the Arecibo sample. JIMENEZ-ESTEBAN F.M., ENGELS D., AGUADO D.S., et al.
2025AJ....170...84B 19       D               7 156 ~ Survey of Oxygen-rich AGB Stars Using the KVN 4 Receiving Bands-SMASTES. I. BAEK H., CHO S.-H., KIM J., et al.

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