V* BK Ori , the SIMBAD biblio

V* BK Ori , the SIMBAD biblio (28 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST16:48:27


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Title First 3 Authors
1919AN....208..245E 63 T                   1 1 0 Neuer Veraenderlicher 18.1919 Orionis =
BD +7 920.
ESCH M.
1919AN....208..277W 63 T                   1 1 0
18.1919 Orionis.
WOLF M.
1965ApJ...142..943S 284 32 Kinematics of the Mira variables. SMAK J.I. and PRESTON G.W.
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.
1978AJ.....83..955B 94 11 High-sensitivity search OH emission from Mira variables. BOWERS P.F. and SINHA R.P.
1978ApJ...220..836F 160 21 A low-detection limit search for OH emission from infrared stars. FIX J.D. and WEISBERG J.M.
1986A&AS...65..607O 5418 387 IRAS catalogues and atlases. Atlas of Low-Resolution Spectra. OLNON F.M., RAIMOND E. (The IRAS Science Team)
1987A&A...175..164B 89 57 SiO maser emission in evolved stars: relation to IR continuum. BUJARRABAL V., PLANESAS P. and DEL ROMERO A.
1988A&A...206..285S 279 60 Criteria for OH maser emission from circumstellar envelopes of oxygen-rich Mira-type red giants. SIVAGNANAM P., LE SQUEREN A.M. and FOY F.
1989A&A...209..165V 176 9 IRAS low resolution spectrograph spectral class and M and S Miras. VARDYA M.S.
1989A&AS...81..323E 189 32 A reference catalogue of maser and thermal emission from circumstellar SiO molecules. ENGELS D. and HESKE A.
1990AJ.....99.1173L 288 111 Emission features in IRAS LRS spectra of Mira variables. LITTLE-MARENIN I.R. and LITTLE S.J.
1994PASJ...46..629T 205 38 Spectral evolution of the H2O maser in late-type stars. TAKABA H., UKITA N., MIYAJI T., 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 11280 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.
2001BAVSR..50...48H 73 T                   3 0 Periodenanderungen beim Mirastern BK Ori. HASSFORTHER B.
2002AcA....52..397P viz 15       D               2893 1175 The All Sky Automated Survey. Catalog of variable stars. I. 0h -6h quarter of the Southern hemisphere. POJMANSKI G.
2004A&A...428..925V 39 12 A photometric pilot study on Sonneberg archival patrol plates. How many ``constant'' stars are in fact long-term variables? VOGT N., KROLL P. and SPLITTGERBER E.
2005AJ....130..776T viz 547 69 Secular evolution in Mira variable pulsations. TEMPLETON M.R., MATTEI J.A. and WILLSON L.A.
2005BAVSM.174....1H 366 0 Beobachtungssergebnisse Bundesdeutsche Arbeitsgemeinschaft fuer Veraenderliche Sterne e.V. HUBSCHER J., LANGE T., PASCHKE A., et al.
1981PZP.....4...85B 433 0 Suggested identifications for infrared sources. BUSCOMBE W.
2012A&A...548A..79A viz 15       D               1 5273 86 The first INTEGRAL-OMC catalogue of optically variable sources. ALFONSO-GARZON J., DOMINGO A., MAS-HESSE J.M., et al.
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 17       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 17       D               1 3874 ~ Long-period high-amplitude red variables in the KELT survey. ARNOLD R.A., McSWAIN M.V., PEPPER J., et al.
2023A&A...674A..15L 19       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.

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