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Gigoyan, K. S., Kostandyan, G. R., Gigoyan, K. K., Zamkotsian, F., Sarkissian, A. (2019) New Carbon Stars Confirmed in the Digitized First Byurakan Survey Database. Astrophysics, 62 (4). 573-577 doi:10.1007/s10511-019-09605-3

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Reference TypeJournal (article/letter/editorial)
TitleNew Carbon Stars Confirmed in the Digitized First Byurakan Survey Database
JournalAstrophysics
AuthorsGigoyan, K. S.Author
Kostandyan, G. R.Author
Gigoyan, K. K.Author
Zamkotsian, F.Author
Sarkissian, A.Author
Year2019 (December)Volume62
Issue4
PublisherSpringer Science and Business Media LLC
DOIdoi:10.1007/s10511-019-09605-3Search in ResearchGate
Generate Citation Formats
Mindat Ref. ID3596698Long-form Identifiermindat:1:5:3596698:8
GUID0
Full ReferenceGigoyan, K. S., Kostandyan, G. R., Gigoyan, K. K., Zamkotsian, F., Sarkissian, A. (2019) New Carbon Stars Confirmed in the Digitized First Byurakan Survey Database. Astrophysics, 62 (4). 573-577 doi:10.1007/s10511-019-09605-3
Plain TextGigoyan, K. S., Kostandyan, G. R., Gigoyan, K. K., Zamkotsian, F., Sarkissian, A. (2019) New Carbon Stars Confirmed in the Digitized First Byurakan Survey Database. Astrophysics, 62 (4). 573-577 doi:10.1007/s10511-019-09605-3
In(2019, December) Astrophysics Vol. 62 (4) Springer Science and Business Media LLC

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Gigoyan, K. S., Mauron, N., Sarkissian, A., Zamkotsian, F., Kostandyan, G. R., Meftah, M., Gigoyan, K. K., Vartanian, R. (2018) New Carbon Stars in the Catalina Catalog of Periodic Variables. Astrophysics, 61 (3). 324-332 doi:10.1007/s10511-018-9539-4
Kostandyan, G., Gigoyan, K. S., Sarkissian, A., Meftah, M., Zamkotsian, F. (2017) New CH Carbon Stars Found in the DFBS. Astrophysics, 60 (2). 300-303 doi:10.1007/s10511-017-9483-8
Gigoyan, K. S., Sarkissian, A., Rossi, C., Russeil, D., Kostandyan, G., Calabresi, M., Zamkotsian, F., Meftah, M. (2017) Investigation of Faint Galactic Carbon Stars from the First Byurakan Spectral Sky Survey. III. Infrared Characteristics. Astrophysics, 60 (1). 70-82 doi:10.1007/s10511-017-9463-z
Gigoyan, K. S., Sarkissian, A., Kostandyan, G. R., Gigoyan, K. K., Meftah, M., Bekki, S., Azatyan, N., Zamkotsian, F. (2023) M dwarfs found in the first Byurakan spectral sky survey database. Gaia EDR3 and TESS data. Some preliminary results. Publications of the Astronomical Society of Australia, 40. doi:10.1017/pasa.2023.20
Gigoyan, K S, Sarkissian, A, Kostandyan, G R, Gigoyan, K K, Meftah, M (2025) Value-added catalogue of late-type stars found in the Digitized First Byurakan Survey data base: third edition. Monthly Notices of the Royal Astronomical Society, 539 (1). doi:10.1093/mnras/staf486
Gigoyan, K. S., Sarkissian, A., Russeil, D., Mauron, N., Kostandyan, G., Vartanian, R., Abrahamyan, H. V., Paronyan, G. M. (2015) Investigation of Faint Galactic Carbon Stars from the First Byurakan Spectral Sky Survey. II. Early-Type Carbon Stars. Astrophysics, 58 (3). 369-379 doi:10.1007/s10511-015-9390-9
Gigoyan, K. S., Russeil, D., Mickaelian, A. M., Sarkissian, A., Avtandilyan, M. G. (2012) New carbon stars found in the Digitized First Byurakan Survey. Astronomy & Astrophysics, 544. doi:10.1051/0004-6361/201219581
Gigoyan, K. S., Sarkissian, A., Russeil, D., Mauron, N., Kostandyan, G., Vartanian, R., Abrahamyan, H. V., Paronyan, G. M. (2014) Investigation of Faint Galactic Carbon Stars from the First Byurakan Spectral sky Survey. Optical Variability. I. N-Type AGB Carbon Stars. K-band Absolute Magnitudes and Distances. Astrophysics, 57 (4). 510-519 doi:10.1007/s10511-014-9354-5
Mauron, N., Gigoyan, K. S., Gigoyan, K. K., Maurin, L. P. A., Kendall, T. R. (2019) Investigation of Long-Period Variables in the Catalina Southern Catalog: New Carbon Stars and False Objects. Astrophysics, 62 (2). 202-209 doi:10.1007/s10511-019-09574-7
Mauron, N., Gigoyan, K. S., Kostandyan, G. R. (2018) New Asymptotic Giant Branch Carbon Stars in the Galactic Halo. Astrophysics, 61 (1). 83-90 doi:10.1007/s10511-018-9517-x
Gigoyan, K. S., Kostandyan, G., Sarkissian, A., Russeil, D. (2013) FBS 0137+400: an N-type semiregular variable carbon star. Astrophysics, 56 (2). 267-270 doi:10.1007/s10511-013-9285-6
 
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