Low-mass star formation in Lynds 1333

M. Kun; S. Nikolić; L. E.B. Johansson; Z. Balog; A. Gáspár

doi:10.1111/j.1365-2966.2006.10698.x

Low-mass star formation in Lynds 1333

M. Kun, S. Nikolić, L. E.B. Johansson, Z. Balog, A. Gáspár

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

1 Scopus citations

Abstract

Medium-resolution optical spectroscopy of the candidate young stellar objects associated with the small, nearby molecular cloud Lynds 1333 revealed four previously unknown classical T Tauri stars, two of which are components of a visual double, and a Class I source, IRAS 02086+7600. The spectroscopic data, together with new V, R_C, I_C photometric and 2MASS J, H, and K_s data allowed us to estimate the masses and ages of the new T Tauri stars. We touch on the possible scenario of star formation in the region. L1333 is one of the smallest and nearest known star-forming clouds, therefore it may be a suitable target for studying in detail the small-scale structure of a star-forming environment.

Original language	English (US)
Pages (from-to)	732-738
Number of pages	7
Journal	Monthly Notices of the Royal Astronomical Society
Volume	371
Issue number	2
DOIs	https://doi.org/10.1111/j.1365-2966.2006.10698.x
State	Published - Sep 2006
Externally published	Yes

Keywords

ISM: clouds
ISM: individual: L1333
Stars: formation
Stars: pre-main-sequence

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1111/j.1365-2966.2006.10698.x

Cite this

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abstract = "Medium-resolution optical spectroscopy of the candidate young stellar objects associated with the small, nearby molecular cloud Lynds 1333 revealed four previously unknown classical T Tauri stars, two of which are components of a visual double, and a Class I source, IRAS 02086+7600. The spectroscopic data, together with new V, RC, IC photometric and 2MASS J, H, and Ks data allowed us to estimate the masses and ages of the new T Tauri stars. We touch on the possible scenario of star formation in the region. L1333 is one of the smallest and nearest known star-forming clouds, therefore it may be a suitable target for studying in detail the small-scale structure of a star-forming environment.",

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AU - Kun, M.

AU - Nikolić, S.

AU - Johansson, L. E.B.

AU - Balog, Z.

AU - Gáspár, A.

PY - 2006/9

Y1 - 2006/9

N2 - Medium-resolution optical spectroscopy of the candidate young stellar objects associated with the small, nearby molecular cloud Lynds 1333 revealed four previously unknown classical T Tauri stars, two of which are components of a visual double, and a Class I source, IRAS 02086+7600. The spectroscopic data, together with new V, RC, IC photometric and 2MASS J, H, and Ks data allowed us to estimate the masses and ages of the new T Tauri stars. We touch on the possible scenario of star formation in the region. L1333 is one of the smallest and nearest known star-forming clouds, therefore it may be a suitable target for studying in detail the small-scale structure of a star-forming environment.

AB - Medium-resolution optical spectroscopy of the candidate young stellar objects associated with the small, nearby molecular cloud Lynds 1333 revealed four previously unknown classical T Tauri stars, two of which are components of a visual double, and a Class I source, IRAS 02086+7600. The spectroscopic data, together with new V, RC, IC photometric and 2MASS J, H, and Ks data allowed us to estimate the masses and ages of the new T Tauri stars. We touch on the possible scenario of star formation in the region. L1333 is one of the smallest and nearest known star-forming clouds, therefore it may be a suitable target for studying in detail the small-scale structure of a star-forming environment.

KW - ISM: clouds

KW - ISM: individual: L1333

KW - Stars: formation

KW - Stars: pre-main-sequence

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Low-mass star formation in Lynds 1333

Abstract

Keywords

ASJC Scopus subject areas

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