The Ages of Optically Bright Subclusters in the Serpens Star-forming Region

Xingyu Zhou; Gregory J. Herczeg; Yao Liu; Min Fang; Michael Kuhn

doi:10.3847/1538-4357/ac704d

The Ages of Optically Bright Subclusters in the Serpens Star-forming Region

Xingyu Zhou, Gregory J. Herczeg, Yao Liu, Min Fang, Michael Kuhn

Research output: Contribution to journal › Article › peer-review

Abstract

The Serpens Molecular Cloud is one of the most active star-forming regions within 500 pc, with over 1000 young stellar objects (YSOs) at different evolutionary stages. The ages of the member stars inform us about the star formation history of the cloud. In this paper, we develop a spectral energy distribution (SED) fitting method for nearby evolved (diskless) young stars from members of the Pleiades to estimate their ages, with a temperature scale adopted from APOGEE spectra. When compared with literature temperatures of selected YSOs in Orion, the SED fits to cool (

Original language	English
Article number	77
Journal	The Astrophysical Journal
Volume	933
DOIs	https://doi.org/10.3847/1538-4357/ac704d
Publication status	Published - 1 Jul 2022

Keywords

Young star clusters
T Tauri stars
Spectral energy distribution
Star forming regions
1833
1681
2129
1565
Astrophysics - Solar and Stellar Astrophysics
Astrophysics - Astrophysics of Galaxies

Access to Document

10.3847/1538-4357/ac704d

https://ui.adsabs.harvard.edu/abs/2022ApJ...933...77Z

Cite this

@article{95e366ac44c94febb76f0f7a104b22b1,

title = "The Ages of Optically Bright Subclusters in the Serpens Star-forming Region",

abstract = "The Serpens Molecular Cloud is one of the most active star-forming regions within 500 pc, with over 1000 young stellar objects (YSOs) at different evolutionary stages. The ages of the member stars inform us about the star formation history of the cloud. In this paper, we develop a spectral energy distribution (SED) fitting method for nearby evolved (diskless) young stars from members of the Pleiades to estimate their ages, with a temperature scale adopted from APOGEE spectra. When compared with literature temperatures of selected YSOs in Orion, the SED fits to cool (",

keywords = "Young star clusters, T Tauri stars, Spectral energy distribution, Star forming regions, 1833, 1681, 2129, 1565, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies",

author = "Xingyu Zhou and Herczeg, {Gregory J.} and Yao Liu and Min Fang and Michael Kuhn",

year = "2022",

month = jul,

day = "1",

doi = "10.3847/1538-4357/ac704d",

language = "English",

volume = "933",

journal = "The Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

}

TY - JOUR

T1 - The Ages of Optically Bright Subclusters in the Serpens Star-forming Region

AU - Zhou, Xingyu

AU - Herczeg, Gregory J.

AU - Liu, Yao

AU - Fang, Min

AU - Kuhn, Michael

PY - 2022/7/1

Y1 - 2022/7/1

N2 - The Serpens Molecular Cloud is one of the most active star-forming regions within 500 pc, with over 1000 young stellar objects (YSOs) at different evolutionary stages. The ages of the member stars inform us about the star formation history of the cloud. In this paper, we develop a spectral energy distribution (SED) fitting method for nearby evolved (diskless) young stars from members of the Pleiades to estimate their ages, with a temperature scale adopted from APOGEE spectra. When compared with literature temperatures of selected YSOs in Orion, the SED fits to cool (

AB - The Serpens Molecular Cloud is one of the most active star-forming regions within 500 pc, with over 1000 young stellar objects (YSOs) at different evolutionary stages. The ages of the member stars inform us about the star formation history of the cloud. In this paper, we develop a spectral energy distribution (SED) fitting method for nearby evolved (diskless) young stars from members of the Pleiades to estimate their ages, with a temperature scale adopted from APOGEE spectra. When compared with literature temperatures of selected YSOs in Orion, the SED fits to cool (

KW - Young star clusters

KW - T Tauri stars

KW - Spectral energy distribution

KW - Star forming regions

KW - 1833

KW - 1681

KW - 2129

KW - 1565

KW - Astrophysics - Solar and Stellar Astrophysics

KW - Astrophysics - Astrophysics of Galaxies

U2 - 10.3847/1538-4357/ac704d

DO - 10.3847/1538-4357/ac704d

M3 - Article

SN - 0004-637X

VL - 933

JO - The Astrophysical Journal

JF - The Astrophysical Journal

M1 - 77

ER -

The Ages of Optically Bright Subclusters in the Serpens Star-forming Region

Abstract

Keywords

Access to Document

Fingerprint

Cite this