HYDROGENE NEUTRE AU VOISINAGE DES RADIOSOURCES GALACTIQUES. RESTE DE SUPERNOVA W28VENGER AP; GOSACHINSKIJ IV; GRACHEV VG et al.1982; ASTR. ZH.; SUN; DA. 1982; VOL. 59; NO 1; PP. 20-26; ABS. ENG; BIBL. 25 REF.Article

W 28. A POSSIBLE ASSOCIATION OF SUPERNOVA REMNANTS AND H II REGIONS.GOUDIS C.1976; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1976; VOL. 40; NO 1; PP. 91-110; BIBL. 1 P. 1/2Article

A DENSE MOLECULAR CLOUD IMPACTED BY THE W28 SUPERNOVA REMNANTWOOTTEN A.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 245; NO 1; PART. 1; PP. 105-114; BIBL. 37 REF.Article

OBSERVATIONS DE W28A₂ EN ONDES CENTIMETRIQUES A L'AIDE DE RATAN-600LIPOVKA NM.1979; PIS'MA ASTR. ZH.; SUN; DA. 1979; VOL. 5; NO 10; PP. 514-516; ABS. ENG; BIBL. 7 REF.Article

COMPARAISON DE DEUX OBSERVATIONS DE DEPLACEMENTS ANORMAUX VERS LE ROUGE OBSERVES AU VOISINAGE DU DISQUE SOLAIRE.DEPAQUIT S; VIGIER JP; PECKER JC et al.1975; C.R. ACAD. SCI., B; FR.; DA. 1975; VOL. 280; NO 5; PP. 113-114; ABS. ANGL.; BIBL. 4 REF.Article

Spectroscopic observations of supernova remnant candidates W 28, CTB 1, and DR 4BOHIGAS, J; RUIZ, M. T; CARRASCO, L et al.Revista Mexicana de Astronomía y Astrofísica. 1983, Vol 8, Num 2, pp 155-161, issn 0185-1101Article

A MAP OF THE OH ABSORPTION IN THE DIRECTION OF W 28.PASTCHENKO MI; SLYSH VI.1974; ASTR. AND ASTROPHYS.; GERM.; DA. 1974; VOL. 35; NO 1; PP. 153-155; BIBL. 9 REF.Article

DO THE W44 AND W28 MOLECULAR CLOUDS SHOW EVIDENCE OF A SHOCK.DE NOYER LK.1983; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1983; VOL. 264; NO 1; PART. 1; PP. 141-151; BIBL. 34 REF.Article

HIGH-RESOLUTION RADIO AND X-RAY OBSERVATIONS OF THE SUPERNOVA REMNANT W28ANDREWS MD; BASART JP; LAMB RC et al.1983; ASTROPHYSICAL JOURNAL; ISSN 0004-637X; USA; DA. 1983; VOL. 266; NO 2; PART. 1; PP. 684-688; BIBL. 19 REF.Article

MOLECULAR CLOUDS NEAR SUPERNOVA REMNANTSSLYSH VI; WILSON TL; PAULS T et al.1980; SYMP.-INT. ASTRON. UNION; ISSN 0074-1809; NLD; DA. 1980; NO 87; PP. 473-478; BIBL. 7 REF.Conference Paper

Far-infrared sources in the vicinity of the supernova remnant W28ODENWALD, S. F; SHIVANANDAN, K; FAZIO, G. G et al.The Astrophysical journal. 1984, Vol 279, Num 1, pp 162-165, issn 0004-637XArticle

The probable identification of two COS-B γ-ray sources with molecular clouds compressed by supernova remnantsPOLLOCK, A. M. T.Astronomy and astrophysics (Berlin. Print). 1985, Vol 150, Num 2, pp 339-342, issn 0004-6361Article

The structure of the faint nebulosity and obscuration toward M8, M20, and W28HARTL, H; MALIN, D. F; MACGILLIVRAY, H. T et al.Astrophysical Letters. 1983, Vol 23, Num 4, pp 193-205, issn 0004-6388Article

Far-infrared photometry of selected sources in the W28 region: M8, W28A2, W28SNR (G6.6 - 0.1), G7.5 + 0.1 and G8.1 + 0.2LIGHTFOOT, J. F; DEIGHTON, D. W; FURNISS, I et al.Monthly Notices of the Royal Astronomical Society. 1984, Vol 208, Num 1, pp 197-213, issn 0035-8711Article