BD-10 4457 , the SIMBAD biblio

BD-10 4457 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST21:46:18

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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
1972A&A....17..385W 449 160 Characteristics of OH emission from infrared stars. WILSON W.J. and BARRETT A.H.
1975AJ.....80.1011H viz 1434 53 Classification of 831 two-micron sky survey sources south of +5 degrees. HANSEN O.L. and BLANCO V.M.
1986A&AS...65..607O 5415 387 IRAS catalogues and atlases. Atlas of Low-Resolution Spectra. OLNON F.M., RAIMOND E. (The IRAS Science Team)
1987ApJ...315..654V 468 41 On the contribution of interstellar extinction to the 10 micron dust feature in OH/IR stars. VOLK K. and KWOK S.
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
1990A&AS...85..875H 111 28 Detection of 51 new 86 GHz SiO, v=1, J=2 ⟶ 1 masers associated with IRAS point sources. HAIKALA L.K.
1990MNRAS.247..549H 65 20 Observations of 43-GHz SiO masers associated with bright IRAS sources. HALL P.J., WRIGHT A.E., TROUP E.R., et al.
1991A&AS...90..327T viz 14       D               1 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.
1991ApJ...368..570S 89 50 IRAS low-resolution spectral observations of the 10 and 18 micron silicate emission features. SIMPSON J.P.
1992A&AS...93..121N viz 514 132 A survey of circumstellar CO emission from a sample of IRAS point sources. NYMAN L.-A., BOOTH R.S., CARLSTROM U., et al.
1992A&AS...93..151F viz 515 106 Near-infrared photometry of a sample of IRAS Point Sources. FOUQUE P., LE BERTRE T., EPCHTEIN N., et al.
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.
1994A&AS..103..107H 170 29 86 GHz SiO, v=1, J=2⟶1 survey of southern IRAS point sources. II. Detection of 74 new maser sources. HAIKALA L.K., NYMAN L.-A. and FORSSTROEM V.
1995PPMtO..14..185H viz 14       D               1 437 0 An atlas of H2O maser observations on the 13.7m radio telescope of Purple Mountain Observatory. HAN F., MAO R.Q., LEI C.-M., et al.
1997ApJ...476..199B 54 189 Aluminum oxide and the opacity of oxygen-rich circumstellar dust in the 12-17 micron range. BEGEMANN B., DORSCHNER J., HENNING T., 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.
1999Ap&SS.262..127K 106 ~ Circumstellar shells of the mass-losing asymptotic giant branch stars: limits for the dust-driven winds. KUCINSKAS A.
2003A&A...409..715W 65 84 Mass-loss from dusty, low outflow-velocity AGB stars. I. Wind structure and mass-loss rates. WINTERS J.M., LE BERTRE T., JEONG K.S., et al.
2003AJ....126..935S 208 22 Infrared colors and variability of evolved stars from COBE DIRBE data. SMITH B.J.
2010ApJS..190..203P viz 15       D               1 2650 25 3.6 years of DIRBE near-infrared stellar light curves. PRICE S.D., SMITH B.J., KUCHAR T.A., et al.
2014ApJS..211...15Y viz 15       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.
2022MNRAS.512.1091S viz 17       D               1 861 5 The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope. SCICLUNA P., KEMPER F., McDONALD I., et al.
2023A&A...674A..15L viz 17       D               1 1720610 15 Gaia Data Release 3 The second Gaia catalogue of long-period variable candidates. LEBZELTER T., MOWLAVI N., LECOEUR-TAIBI I., et al.
2024ApJS..270...13F viz 18       D               1 865 ~ Systematic Search for Water Fountain Candidates Using the Databases of Circumstellar Maser Sources. FAN H., NAKASHIMA J.-I., ENGELS D., et al.

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