[FLG2003] eps Cha 7 , the SIMBAD biblio

[FLG2003] eps Cha 7 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST06:07:20

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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
2003ApJ...599.1207F 60 82 The ε Chamaeleontis young stellar group and the characterization of sparse stellar clusters. FEIGELSON E.D., LAWSON W.A. and GARMIRE G.P.
2004ApJ...608..809G 26 74 The environment of the optically brightest Herbig Ae star, HD 104237. GRADY C.A., WOODGATE B., TORRES C.A.O., et al.
2004ApJ...614..221S 41 37 New perspectives on the X-ray emission of HD 104237 and other nearby Herbig Ae/Be stars from XMM-newton and Chandra. SKINNER S.L., GUDEL M., AUDARD M., et al.
2004ApJ...616.1033L 22 34 A survey for low-mass stars and brown dwarfs in the η Chamaeleontis and ε Chamaeleontis young associations. LUHMAN K.L.
2006A&A...457..223S 42 75 On the origin of the X-ray emission from Herbig Ae/Be stars. STELZER B., MICELA G., HAMAGUCHI K., et al.
2007MNRAS.381.1569H 352       D S   X   F     8 14 4 Establishing the nature of companion candidates to X-ray-emitting late B-type stars. HUBRIG S., MARCO O., STELZER B., et al.
2008MNRAS.389.1461L 467       D     X C       12 59 10 Spectrophotometric properties of pre-main-sequence stars: the εChamaeleontis cluster. LYO A.-R., LAWSON W.A. and BESSELL M.S.
2008ApJ...687..579T 15 14 X-ray emission from young stellar objects in the ε Chamaeleontis group: the Herbig Ae star HD 104237 and associated low-mass stars. TESTA P., HUENEMOERDER D.P., SCHULZ N.S., et al.
2009A&A...508..833D viz 15       D               1 372 134 Search for associations containing young stars (SACY). III. Ages and Li abundances. DA SILVA L., TORRES C.A.O., DE LA REZA R., et al.
2011A&A...532A..10M viz 131       D     X         4 216 40 RACE-OC project: rotation and variability in the ε Chamaeleontis, Octans, and Argus stellar associations. MESSINA S., DESIDERA S., LANZAFAME A.C., et al.
2012ApJS..201...11K viz 116           X   F     2 101 25 Mid-infrared spectral variability atlas of young stellar objects. KOSPAL A., ABRAHAM P., ACOSTA-PULIDO J.A., et al.
2013A&A...549A..15F 133       D     X         4 102 28 Young stars in ε Chamaleontis and their disks: disk evolution in sparse associations. FANG M., VAN BOEKEL R., BOUWMAN J., et al.
2013A&A...551A..46L viz 94       D   O   C       3 248 21 Proper motions of young stars in Chamaeleon. I. A virtual observatory study of spectroscopically confirmed members. LOPEZ MARTI B., JIMENEZ-ESTEBAN F., BAYO A., et al.
2013MNRAS.435.1325M viz 796       D     X C       20 99 50 Re-examining the membership and origin of the ε Cha association. MURPHY S.J., LAWSON W.A. and BESSELL M.S.
2014AJ....148...47H                   Z 77 21 A CO survey in planet-forming disks: characterizing the gas content in the epoch of planet formation. HALES A.S., DE GREGORIO-MONSALVO I., MONTESINOS B., et al.
2017AJ....154..195B viz 16       D               3 59 2 New binaries in the ε Cha association. BRICENO C. and TOKOVININ A.
2018ApJ...856...23G viz 16       D               1 1601 367 BANYAN. XI. The BANYAN Σ multivariate Bayesian algorithm to identify members of young associations with 150 pc. GAGNE J., MAMAJEK E.E., MALO L., et al.
2021A&A...645A..30Z viz 17       D               2 431 20 Search for associations containing young stars (SACY). VIII. An updated census of spectroscopic binary systems exhibiting hints of non-universal multiplicity among their associations. ZUNIGA-FERNANDEZ S., BAYO A., ELLIOTT P., et al.
2021AJ....161...87D viz 409       D     X         10 81 ~ Gaia-based isochronal, kinematic, and spatial analysis of the ε Cha Association. DICKSON-VANDERVELDE D.A., WILSON E.C. and KASTNER J.H.
2021AJ....162...28V viz 17       D               1 661 47 A stellar mass dependence of structured disks: a possible link with exoplanet demographics. VAN DER MAREL N. and MULDERS G.D.
2023AJ....165..165T 112       D     X         3 14 ~ Dynamics of Four Triple Systems. TOKOVININ A.

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