IRAS 17482-2501 , the SIMBAD biblio

IRAS 17482-2501 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST14:14:01


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Title First 3 Authors
1988A&AS...76..317P viz 396 73 Possible new planetary nebulae in the IRAS point source catalogue. PREITE-MARTINEZ A.
1989A&AS...78..399T 574 131 A catalogue of stellar 1612 MHz maser sources. TE LINTEL HEKKERT P., VERSTEEGE-HANSEL H.A., HABING H.J., et al.
1997A&AS..122...79S viz 14       D               1 390 131 The ATCA/VLA OH 1612 MHz survey. I. Observations of the Galactic bulge region. SEVENSTER M.N., CHAPMAN J.M., HABING H.J., et al.
2002AJ....123.2788S 62 26 OH-selected AGB and Post-AGB objects. II. Blue versus red evolution off the asymptotic giant branch. SEVENSTER M.N.
2007ApJ...658.1096D viz 15       D               1 104 40 H2O maser observations of candidate post-AGB stars and discovery of three high-velocity water sources. DEACON R.M., CHAPMAN J.M., GREEN A.J., et al.
2009A&A...501.1207R 15       D               2 171 16 Searching for heavily obscured post-AGB stars and planetary nebulae. I. IRAS candidates with 2MASS Psc counterparts. RAMOS-LARIOS G., GUERRERO M.A., SUAREZ O., et al.
2012A&A...545A..20R 170       D       C F     5 176 27 Searching for heavily obscured post-AGB stars and planetary nebulae. II. Near-IR observations of IRAS sources. RAMOS-LARIOS G., GUERRERO M.A., SUAREZ O., et al.
2014ApJS..211...15Y viz 16       D               2 314 17 SiO and H2 O maser survey toward post-asymptotic giant branch and asymptotic giant branch stars. YOON D.-H., CHO S.-H., KIM J., et al.
2015A&A...578A.119G viz 16       D               2 142 10 A search for water maser emission toward obscured post-AGB star and planetary nebula candidates. GOMEZ J.F., RIZZO J.R., SUAREZ O., et al.
2018ApJS..239...15Q viz 41           X         1 371 4 Accurate OH maser positions. II. The Galactic Center region. QIAO H.-H., WALSH A.J., BREEN S.L., et al.
2021MNRAS.506.5223J 17       D               1 221 15 Binary central stars of planetary nebulae identified with Kepler/K2. JACOBY G.H., HILLWIG T.C., JONES D., et al.

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