The near-ultraviolet luminosity function of young, early M-type dwarf stars

Planets orbiting within the close-in habitable zones of M dwarf stars will be exposed to elevated high-energy radiation driven by strong magnetohydrodynamic dynamos during stellar youth. Near-ultraviolet (NUV) irradiation can erode and alter the chemistry of planetary atmospheres, and a quantitative...

Descripción completa

Guardado en:

Detalles Bibliográficos
Autores principales:	Buccino, Andrea Paola, Mauas, Pablo J.D., Petrucci, Romina Paola
Publicado:	2015
Materias:	Binaries: Close Stars: Activity Stars: Late-type Stars: Luminosity function, mass function
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v798_n1_p_Ansdell http://hdl.handle.net/20.500.12110/paper_0004637X_v798_n1_p_Ansdell
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

The near-ultraviolet luminosity function of young, early M-type dwarf stars
por: Ansdell, M., et al.

The β Pictoris association: Catalog of photometric rotational periods of low-mass members and candidate members
por: Buccino, Andrea Paola, et al.
Publicado: (2017)

White dwarf luminosity and mass functions from sloan digital sky survey spectra
por: DeGennaro, Steven, et al.
Publicado: (2008)

Limits on the neutrino magnetic dipole moment from the luminosity function of hot white dwarfs
por: Miller Bertolami, Marcelo Miguel
Publicado: (2014)

Revisiting the luminosity function of single halo white dwarfs
por: Cojocaru, Ruxandra, et al.
Publicado: (2015)

Chromospheric models of dwarf M stars
por: Mauas, P.J.D., et al.

Detailed photometric analysis of young star groups in the galaxy NGC 300
por: Rodríguez, María Jimena, et al.
Publicado: (2016)

The β Pictoris association: Catalog of photometric rotational periods of low-mass members and candidate members
por: Messina, S., et al.

The β Pictoris association low-mass members: Membership assessment, rotation period distribution, and dependence on multiplicity
por: Messina, S., et al.

OWN Survey: A spectroscopic monitoring of Southern Galactic O and WN-type stars
por: Barbá, Rodolfo Héctor, et al.
Publicado: (2016)

Chromospheric models of dwarf M stars
Publicado: (1997)

The massive Wolf-Rayet binary LSS 1964 (=WR 29)
por: Gamen, Roberto Claudio, et al.
Publicado: (2009)

Grids of white dwarf evolutionary models with masses from M= 0.1 to 1.2 M☉
por: Benvenuto, Omar Gustavo, et al.
Publicado: (1999)

The β Pictoris association low-mass members: Membership assessment, rotation period distribution, and dependence on multiplicity
Publicado: (2017)

The Gaia DR2 halo white dwarf population: the luminosity function, mass distribution, and its star formation history
por: Torres, Santiago, et al.
Publicado: (2021)

A peculiar interacting Be star binary in the Small Magellanic Cloud
por: Mennickent, Ronald E., et al.
Publicado: (2018)

The young open cluster Markarian 50
por: Baume, Gustavo, et al.
Publicado: (2004)

Identification and analysis of the young population in the starburst galaxy NGC 253
por: Rodríguez, María Jimena, et al.
Publicado: (2018)

Photometric study of the young open cluster NGC 3293
por: Baume, Gustavo Luis, et al.
Publicado: (2003)

The contribution of oxygen-neon white dwarfs to the MACHO content of the Galactic halo
por: Camacho, J., et al.
Publicado: (2007)

The Na i D resonance lines in main-sequence late-type stars
por: Díaz, R.F., et al.

Binary evolution leading to the formation of the very massive neutron star in the J0740+6620 binary system
por: Echeveste, Maite, et al.
Publicado: (2020)

RW Doradus: a solar-type shallow contact binary with a new orbital period investigation
por: Sarotsakulchai, Thawicharat, et al.
Publicado: (2019)

Age of the magnetically active WW Psa and TX Psa members of the β Pictoris association
por: Messina, S., et al.

On the evolutionary status of Be stars : I. Field Be stars near the Sun
por: Zorec, J., et al.
Publicado: (2005)

Confirmation and revision on the orbital period change of the possible type Ia supernova progenitor V617 Sagittarii
por: Shi, Guang, et al.
Publicado: (2014)

SEMI-EMPIRICAL MODELING of the PHOTOSPHERE, CHROMOPSHERE, TRANSITION REGION, and CORONA of the M-DWARF HOST STAR GJ 832
por: Fontenla, J.M., et al.

Evolutionary states of the two shortest period O-type overcontact binaries V382 Cyg and TU Mus
por: Qian, S. B., et al.
Publicado: (2007)

Building reliable models of M dwarf chromospheres: The spectral diagnostics
por: Mauas, P.J.D.

NGC 2571: An intermediate-age open cluster with a White Dwarf candidate
por: Giorgi, Edgard Ervar Salvador, et al.
Publicado: (2002)

On the multiplicity of the zero-age main-sequence O star Herschel 36
por: Arias, Julia Inés, et al.
Publicado: (2010)

SDSS J001641-000925: The first stable red dwarf contact binary with a close-in stellar companion
por: Qian, S. B., et al.
Publicado: (2015)

NGC 2401: A template of the young population of the Norma-Cygnus arm in the Third Galactic Quadrant
por: Baume, Gustavo Luis, et al.
Publicado: (2006)

Hodge 53-47: An early O-type double-lined binary in the Small Magellanic Cloud
por: Morrell, Nidia Irene, et al.
Publicado: (2003)

Building reliable models of M dwarf chromospheres: The impact of the usual assumptions
por: Falchi, A., et al.

Is WX CEN a possible type Ia supernova progenitor with wind-driven mass transfer?
por: Qian, S.-B., et al.
Publicado: (2013)

White dwarf–main-sequence binaries from Gaia EDR3: the unresolved 100 pc volume-limited sample
por: Rebassa Mansergas, Alberto, et al.
Publicado: (2021)

SDSS DR7 white dwarf catalog
por: Kleinman, S. J., et al.
Publicado: (2013)

The Evolution of the Supersoft X-Ray Source WX Cen Dominated by Magnetic Wind
por: Zang, Lei, et al.
Publicado: (2023)

The Na i D resonance lines in main-sequence late-type stars
Publicado: (2007)