IRAS 19214+1458 , the SIMBAD biblio

IRAS 19214+1458 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST15:20:09

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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
1991A&A...246..249P 259 201 Water masers associated with dense molecular clouds and ultracompact HII regions. PALLA F., BRAND J., CESARONI R., et al.
1994ApJ...427..857H 48 20 An analysis of IRAS-identified HII regions and their radio properties. HUGHES V.A. and MacLEOD G.C.
1995A&AS..110...81V viz 562 69 New detections of 51-60A+-methanol masers towards IRAS sources. VAN DER WALT D.J., GAYLARD M.J. and MacLEOD G.C.
1995MNRAS.276...57C viz 1004 53 IRAS-selected Galactic star-forming regions. II. Water maser detections in the extended sample. CODELLA C., PALUMBO G.G.C., PARESCHI G., et al.
1996A&AS..115...81B viz 14       D               1 1472 529 A CS(2-1) survey of IRAS point sources with color characteristics of ultra-compact HII regions. BRONFMAN L., NYMAN L.-A. and MAY J.
1996ApJS..107..239T viz 1940 54 A Westerbork synthesis radio telescope 327 MHz survey of the galactic plane. TAYLOR A.R., GOSS W.M., COLEMAN P.H., et al.
1999A&AS..134..115S viz 411 83 The Medicina survey of methanol masers at 6.7GHz. SLYSH V.I., VAL'TTS I.E., KALENSKII S.V., et al.
2000A&AS..143..269S viz 1601 191 A survey of the 6.7 GHz methanol maser emission from IRAS sources. I. Data. SZYMCZAK M., HRYNEK G. and KUS A.J.
2010A&A...517A..56F 15       D               1 307 67 Class I and class II methanol masers in high-mass star-forming regions. FONTANI F., CESARONI R. and FURUYA R.S.
2018A&A...617A..67S 1019       D     X         26 87 6 Bipolar H II regions. II. Morphologies and star formation in their vicinities. SAMAL M.R., DEHARVENG L., ZAVAGNO A., et al.

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