IRAS 19396+2338 , the SIMBAD biblio

IRAS 19396+2338 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST16:44:14

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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
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
1990ApJ...362..634L 493 91 New OH/IR stars from color-selected IRAS sources. II. An unbiased 1612 MHz survey. LEWIS B.M., EDER J. and TERZIAN Y.
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.
2006AJ....132..489L 21 2 On modeling the near-infrared two-color locus of OH/IR stars with a constant dM/dt. LEWIS B.M.
2013A&A...549A.130V viz 15       D               1 286 27 An analysis of star formation with Herschel in the Hi-GAL survey. I. The science demonstration phase fields. VENEZIANI M., ELIA D., NORIEGA-CRESPO A., 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.
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.
2025ApJ...978..114X 19       D               3 395 ~ A Search for Asymmetric Kinematic Components in Circumstellar Envelopes Using OH Main Line Masers. XIE J.-Y., NAKASHIMA J.-I. and ZHANG Y.

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