LBN 140.77-01.42 , the SIMBAD biblio

LBN 140.77-01.42 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST05:40:33


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Title First 3 Authors
1989AJ.....98.2210G 70 T                   1 9 5 Studies of two Lynds bright nebulae:
LBN 140.77-1.42, a remarkable thermal ridge, and LBN 139.57+2.70, a radio and infrared partial ring.
GREEN D.A.
1989BAAS...21..762G 70 T                   1 1 0
LBN 140.77-1.42, a large thermal ridge.
GREEN D.A.
2001PASP..113..872K 3 4 A fast technique for the creation of large-scale high-resolution IRAS (HIRES) beam-matched images. KERTON C.R. and MARTIN P.G.
2003AJ....125.3145T viz 7 23 507 The Canadian galactic plane survey. TAYLOR A.R., GIBSON S.J., PERACAULA M., et al.
2003ApJ...595..880K 36   K                 45 4 Three Lynds bright nebulae. KARR J.L. and MARTIN P.G.
2003JRASC..97Q..32K 12 0 A multi-wavelenght study of star formation around H II regions. (Thesis abstract) KARR J.
2007ApJ...659..426D 39 14 Infrared excess sources in the Canadian Galactic Plane Survey. DOUGLAS K.A. and TAYLOR A.R.
2007BaltA..16..327S viz 62 13 Young stars in the Camelopardalis dust and molecular clouds. II. Infrared objects. STRAIZYS V. and LAUGALYS V.
2010A&A...515A..64G 467       D     X C       12 41 58 A sino-german λ6 cm polarization survey of the galactic plane. II. The region from 129° to 230° longitude. GAO X.Y., REICH W., HAN J.L., et al.
2010BaltA..19....1S viz 49 3 Young stars in the Camelopardalis dust and molecular clouds. VI. YSOs verified by Spitzer and Akari infrared photometry. STRAIZYS V. and KAZLAUSKAS A.
2017MNRAS.467.4631H 79           X         2 17 15 The Fan Region at 1.5 GHz - I. Polarized synchrotron emission extending beyond the Perseus Arm. HILL A.S., LANDECKER T.L., CARRETTI E., et al.
2021MNRAS.506.6081D 485   K A     X         12 15 3 Lynds Bright Nebulae: sites of possible twisted filaments and ongoing star formation. DEWANGAN L.K., DHANYA J.S., BHADARI N.K., et al.
2025ApJ...991..118T 47           X         1 37 ~ A Systematic Search for Main-sequence Dipper Stars Using the Zwicky Transient Facility. TZANIDAKIS A., DAVENPORT J.R.A., CAPLAR N., et al.

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