IRAS 19124+1106 , the SIMBAD biblio

IRAS 19124+1106 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST06:17:47

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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
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.
1993MNRAS.261..783S 280 89 Detection of 35 new 5 1 -6 0 A+ -methanol masers towards IRAS sources. SCHUTTE A.J., VAN DER WALT D.J., GAYLARD M.J., et al.
1995MNRAS.276...57C viz 1003 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 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 4047 54 A Westerbork synthesis radio telescope 327 MHz survey of the galactic plane. TAYLOR A.R., GOSS W.M., COLEMAN P.H., et al.
1998A&A...340L..47R 36   K                 9 24 The surroundings of the superluminal source GRS 1915+105. RODRIGUEZ L.F. and MIRABEL I.F.
1998NewAR..42..649R 10 4 Large studies of the surroundings of GRS 1915+105. RODRIGUEZ L.F. and MIRABEL I.F.
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.
2000AcApS..20..383W 67 2 Searches for massive molecular cloud cores with CO isotopes. WU Y.-F., WU J.-W., WANG J.-Z., et al.
2001A&A...366.1035C 37   K                 8 26 A search for possible interactions between ejections from GRS 1915+105 and the surrounding interstellar medium. CHATY S., RODRIGUEZ L.F., MIRABEL I.F., et al.
2001A&A...367..613O 12 2 An attempt to identify the extended synchrotron structure associated with the micro-quasar GRS 1915+105. OSTROWSKI M. and FUERST E.
2001A&A...380..665W viz 114 21 A search for massive dense cores with 13CO [1]J = 1-0 line. WU Y., WU J. and WANG J.
2004ApJ...612..332K 39   K                 6 52 Revision of the properties of the GRS 1915+105 jets: clues from the large-scale structure. KAISER C.R., GUNN K.F., BROCKSOPP C., et al.
2005MNRAS.360..825Z 2 7 49 GRS 1915+105: the distance, radiative processes and energy-dependent variability. ZDZIARSKI A.A., GIERLINSKI M., RAO A.R., et al.
2008A&A...484..435A 38           X         1 21 18 Discovery of very-high-energy γ-ray emission from the vicinity of PSR J1913+1011 with HESS. AHARONIAN F., AKHPERJANIAN A.G., BARRES DE ALMEIDA U., et al.
2009AJ....138.1380M viz 15       D               1 204 10 Looking through the Galactic Plane: imaging cold dust toward l = 44°. MATTHEWS H., KIRK H., JOHNSTONE D., et al.
2009A&A...508.1135H 114           X         3 12 11 HESS upper limits on very high energy gamma-ray emission from the microquasar GRS 1915+105. HESS COLLABORATION, ACERO F., AHARONIAN F., et al.
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.
2010ApJ...723..915R viz 38           X         1 49 7 The BLAST view of the star-forming region in Aquila (l = 45°, b = 0°). RIVERA-INGRAHAM A., ADE P.A.R., BOCK J.J., et al.
2011A&A...532A.127D viz 15       D               1 80 8 A H2CO and H110α survey of H II regions with the 25-m radio telescope of Nanshan station. DU Z.M., ZHOU J.J., ESIMBEK J., et al.
2014ApJ...796....2R 85           X         2 14 187 A parallax distance to the microquasar GRS 1915+105 and a revised estimate of its black hole mass. REID M.J., McCLINTOCK J.E., STEINER J.F., et al.
2018MNRAS.475..448T 576       S   X C F     11 31 7 Mapping jet-ISM interactions in X-ray binaries with ALMA: a GRS 1915+105 case study. TETARENKO A.J., FREEMAN P., ROSOLOWSKY E.W., et al.
2021ApJ...923..106Z 87           X         2 13 ~ Fermi-LAT detection of extended gamma-ray emission in the vicinity of SNR G045.7-00.4: evidence of escaping cosmic rays interacting with the surrounding molecular clouds. ZHANG H.-M., LIU R.-Y., SU Y., et al.

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