V* AH Oph , the SIMBAD biblio

V* AH Oph , the SIMBAD biblio (25 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST20:37:04


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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.
1983A&AS...54..405C 53 26 A search for water vapor masers associated with infrared sources. CROCKER D.A. and HAGEN W.
1983ApJS...53..413G viz 744 45 The stellar component of the galaxy as seen by the AFGL Infrared Sky Survey. GRASDALEN G.L., GEHRZ R.D., HACKWELL J.A., et al.
1988A&AS...76..445C 366 96 A catalogue of H2O maser sources north of delta = -30. CESARONI R., PALAGI F., FELLI M., et al.
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
1989AJ.....97.1089B 76 29 Single-dish and interferometer measurements of water-maser polarization. BARVAINIS R. and DEGUCHI S.
1990A&AS...84..179C 408 163 The Arcetri atlas of H2O maser sources. COMORETTO G., PALAGI F., CESARONI R., et al.
1991ApJS...77..607V 501 86 New low-resolution spectrometer spectra for IRAS sources. VOLK K., KWOK S., STENCEL R.E., et al.
1993A&AS..101..153P viz 761 132 Classification and statistical properties of galactic H2O masers. PALAGI F., CESARONI R., COMORETTO G., et al.
1995A&AS..111..237L viz 241 25 Mainline OH detection rates from blue circumstellar shells. LEWIS B.M., DAVID P. and LE SQUEREN A.M.
1997ApJS..112..557K viz 11276 205 Classification and identification of IRAS sources with low-resolution spectra. KWOK S., VOLK K. and BIDELMAN W.P.
2000MNRAS.317..460F viz 848 53 Mira kinematics from Hipparcos data: a Galactic bar to beyond the Solar circle. FEAST M.W. and WHITELOCK P.A.
2002AcA....52..397P viz 14       D               2893 1175 The All Sky Automated Survey. Catalog of variable stars. I. 0h -6h quarter of the Southern hemisphere. POJMANSKI G.
2004AJ....128.2965W viz 15       D               1 8686 106 Identifying red variables in the Northern Sky Variability Survey. WOZNIAK S.J., WILLIAMS P.R., VESTRAND W.T., et al.
2008PASJ...60.1077S 15       D               3 247 24 Statistical properties of stellar H2O masers — results of three-year single-dish observations with the VERA Iriki telescope. SHINTANI M., IMAI H., ANDO K., et al.
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.
2013AJ....145...22K viz 15       D               6 154 12 Simultaneous observations of SiO and H2O masers toward known stellar H2O maser sources. KIM J., CHO S.-H. and KIM S.J.
2014AJ....147...22K viz 15       D               1 340 11 Statistical studies based on simultaneous SiO and H2 O maser surveys toward evolved stars. KIM J., CHO S.-H. and KIM S.J.
2016ApJS..227....6V viz 16       D               1 2892 2 Determination of pulsation periods and other parameters of 2875 stars classified as Mira in the All Sky Automated Survey (ASAS). VOGT N., CONTRERAS-QUIJADA A., FUENTES-MORALES I., et al.
2017ARep...61...80S viz 16       D               7150 446 General catalogue of variable stars: Version GCVS 5.1 SAMUS N.N., KAZAROVETS E.V., DURLEVICH O.V., et al.
2019MNRAS.486.1907J viz 16       D               1 8966 183 The ASAS-SN catalogue of variable stars - II. Uniform classification of 412 000 known variables. JAYASINGHE T., STANEK K.Z., KOCHANEK C.S., et al.
2020ApJS..247...44A viz 16       D               1 3874 ~ Long-period high-amplitude red variables in the KELT survey. ARNOLD R.A., McSWAIN M.V., PEPPER J., 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.
2025A&A...700A.187U viz 19       D               1 3121 ~ A population analysis of Galactic Miras with light-curve asymmetries. UTTENTHALER S. and MERCHAN-BENITEZ P.

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